Galaxy of the Month Archive 2023

In this series of articles we draw your attention to galaxies particularly worthly of an observer's time.

• NGC 1507 in Eridanus

  December 2023 - Galaxy of the Month

  With the winter clusters and nebulae season approaching I thought for this month I would try the edge on galaxy NGC 1507 in Eridanus for the GOM. NGC 1507 was first discovered by William Herschel in January 1785 and he described it as very faint.

  It is classified as a barred spiral (SB(s)m pec) and if its distance is about 40 million light-years then it is a small galaxy at perhaps 45,000 light-years in diameter. It does seem a little distorted and from the colours would appear to have a lot of star formation going on, including some very large star clusters. NGC 1507 appears to have no distinct nucleus. It was included in Markarians catalogue of blue sources as Mrk 1080. If the galaxy has been distorted by a merger or interaction this would be odd as the galaxy appears to lie in a void with no other galaxies nearby. There is a nice amateur image showing its blobby nature on Gary Imm's AstroBin. Unfortunately, there does not seem to be much other research on this object.

  Observationally NGC 1507 appears in the Astronomical League's Herschel II list. It does arise above the 30 degree altitude line as seen from the southern UK so should be visible but, as always with this type of galaxy, observe it when it is on or near the meridian. As it is quite small I would suggest a medium to high power when observing it.

  Steve Gottlieb records it as being fairly faint with a 13.1” and the The Night Sky Observer's Guide (NSOG) Vol 1 suggests that it should be visible in 20-25cm telescopes as a faint streak. They also suggest that 30-37cm should show some sign of mottling, however I suspect that under typical UK skies this may require 40cm or more to see as most of the observations in the NSOG were made in high dry sites. Luginbuhl and Skiff (L&S) suggests that it can just be seen in 15cm, although again this was from a premium observing site. They also suggest that 30cm should show some of the condensations in the galaxy.

  Owen Brazell - Galaxy Section Director

• NGC 777 in Triangulum

  November 2023 - Galaxy of the Month

  It is becoming harder to find interesting galaxies that are not too faint to feature in the GOM blog. This month I have chosen the pair of galaxies NGC 777 and NGC 778 in Triangulum.

  NGC 777 was discovered by William Herschel in 1784 but the much fainter NGC 778 had to wait until 1866 when it was discovered by Safford using an 18” refractor at Dearborn observatory in the US, although it was independently rediscovered by Stephan in 1875 using the 30” silver of glass reflector at Marseille. Safford did not publish his observations until 1887, after the NGC was completed.

  NGC 777 is an elliptical galaxy, classified as E1, with a weak active nucleus of the LINER or Seyfert 2 class. The nucleus shows as a bright X-Ray source. It may also be an outlying member of the cluster Abell 262. It lies at a distance of perhaps 187 million light-years. NGC 777 and 778 may form a non-interacting pair. NGC 777 is also included as part of a group of galaxies catalogued as LGG 42 which has 13 galaxies involved including NGC 750, NGC 751, NGC 761, NGC 777, NGC 783, NGC 785 and NGC 789, although interestingly not NGC 778.

  NGC 778 has been classified as an S0, i.e. a lenticular galaxy and according to NED lies much further away than NGC 777 so they may just be an optical pair. It has also been classified as SAB(s)a, which fits with observations with the GALEX satellite in the UV suggest that there may be a ring of star formation in NGC 778 which would be at odds with its lenticular classification. The SDSS image also shows the suggestion of a bar and spiral arms. There are suggestions that NGC 778 may also be a starburst or Seyfert galaxy. NGC 777 just shows a bright core in the UV.

  The The Night Sky Observer's Guide (NSOG) Vol 1 suggests that the pair should be visible in 12-14in (30-35cm) scopes as a faint pair. NGC 777 should be relatively easy and NGC 778 shows as a bright nucleus with a fainter halo. I suspect that as usual from the more polluted skies of the UK that it may well require 40cm to show the same views. Mark Stuarts observation of NGC 777 with a 40cm show it to be faint but there is no mention of him seeing NGC 778.

  Owen Brazell - Galaxy Section Director

• NGC 783 in Triangulum

  October 2023 - Galaxy of the Month

  The GOM this month is going to be a bit of a challenge as it is the faint pair of galaxies around NGC 783 in Triangulum.

  NGC 783 and NGC 785 were discovered by Edouard Stephan in October 1869 using the 31” silver on glass reflector designed by Foucault in Marseille. This telescope was mounted outside and uncovered which tells of the normal good weather there (see the list of objects he found with this telescope on Wolfgang Steinicke's website). He described them as eF which suggests they are going to be a challenge for observers.

  

  Barnard later independently rediscovered these objects in the 1890’s but his reported positions were not very good and when he communicated his observations to Dreyer he were thought that Barnard had discovered two new objects and added them to the NGC supplement as IC 1765 and IC 1766. It was later shown however that these objects are the same as NGC 783 and NGC 785. It is worth noting that some software packages still link IC 1766 to the very faint galaxy PGC 7655, which is definitely not the galaxy Barnard saw.

  Both NGC 783 and NGC 783 are involved in a group of perhaps 13 galaxies called LGG 42, which contains a further 5 NGC galaxies in NGC 750, NGC 751, NGC 761, NGC 777 and NGC 789. The group lies at a distance of perhaps 73 Mpc (238 million light-years away) and is often known as the NGC 777 group.

  NGC 783 is a spiral galaxy with an active nucleus which shows up well in the UV and NGC 783 was subsequently catalogued by Markarian as part of his blue galaxies listings as Mrk 1171. The excess UV light appears to come from a starburst region in the centre of the galaxy, although GALEX observations in the UV suggest that there is a lot of star formation going on in the spiral arms as well. NGC 785 on the other hand is a lenticular galaxy. Although close together on the sky NGC 783 and 785 do not appear to form a physical pair and there are no signs of interactions between them.

  The type Ia supernova SN 2004fz was independently discovered in NGC 783 by the UK amateurs Tom Boles and Ron Arbour. It never became very bright however reaching perhaps 15th magnitude at best, not surprising given the distance to the galaxies which is thought to be about 59Mpc for NGC 783, although other measurements give about 73 Mpc, and perhaps 69 Mpc for NGC 785.

  The pair is also part of a nice chain of galaxies going from NGC 777 to NGC 789 and NGC 798 (which does not appear to be part of the group). It covers about 50’ on the sky.

  As might be expected there are not many visual observations of this pair but the The Night Sky Observer's Guide (NSOG) Vol. 1 suggests that 30-35cm aperture telescopes will be needed to see NGC 783 and perhaps 40-45cm for NGC 785. I suspect from the typical murky UK skies that you will need to use medium to high power to bring the pair out. Luginbuhl and Skiff (L&S) suggest that NGC 783 is faintly visible in 15cm but a 30cm is required to see a very faint smudge of NGC 785. Those observations were made at a high, dry site however.

  Owen Brazell - Galaxy Section Director

• NGC 7603 in Pisces

  September 2023 - Galaxy of the Month

  As the galaxy fields of autumn roll around, I have chosen NGC 7603, also known as Arp 92, in Pisces for the galaxy of the month. First discovered in 1864 by Albert Marth using William Lassell’s 48” speculum metal mirror telescope from Malta.

  Arp included it in his group of spiral galaxies with an elliptical companion. NGC 7603 appears to be interacting with the small elliptical galaxy PGC 71041 nearby, indeed there appears to be a filament connecting the two galaxies. Arp 92 is at the centre of various controversies about cosmological redshifts due to the fact there are two quasars involved with the filament, one at either end, note the dots in the accompanying SDSS image, as well which Arp and Hoyle took to mean they were connected and thus quasars were not at cosmological distances.

  NGC 7603 itself is a distorted spiral galaxy. It seems that occasionally PGC 71041 is also known as NGC 7603B. NGC 7603 is classified as a Seyfert class 1 AGN, although its type seems to have varied over the last 20 years or so due to changes in its spectrum. NGC 7603 is also a very strong blue source catalogued as Mrk 530.

  There are however issues with PGC 71041 being the cause of the interaction as it appears to be nearly twice as far away than NGC 7603. The fact that the spiral arm/filament overlies it appears to be totally coincidental. One other possible candidate for casing the disruption is the barred spiral NGC 7589 which appears to be at the same distance as NGC 7603. It is also possible that the plumes from NGC 7603 are the result of a merger event rather than an interaction.

  There do not seem to be any high-quality images of Arp 92 taken by the HST, but there is one image on Wikipedia. This is a relatively raw/ unprocessed Hubble image as evidenced by all the cosmic ray streaks.

  NGC 7603 would appear to lie at a distance of about 127 Mpc. It was also included in the extended VV catalogue of interacting galaxies as VV 1975.

  It is interesting that given the usual Arp mania there are no observations of Arp 92 in The Night Sky Observer's Guide (NSOG). I note that both Steve Gottlieb and Alvin Huey felt that NGC 7603 was not too hard to find in their large instruments but the companion was very faint in 50cm class telescopes and not surprisingly no spiral structure was seen. Both NGC 7603 and NGC 7589 should appear in the same field with a medium power eyepiece, however as both are quite faint it is probably worth using the highest power eyepiece you can that fits them both in the same field to find them. In Steve Gottlieb's complete NGC observations (on Adventures in Deep Space) he also has observations of the pair with a 48” Dobsonian.

  Owen Brazell - Galaxy Section Director

• NGC 7013 in Cygnus

  August 2023 - Galaxy of the Month

  Moving into August we are now in the Milky Way season and galaxies are becoming harder to find. For this month I have chosen the little observed galaxy NGC 7013 in Cygnus (near the border with Pegasus) as the galaxy of the month. First discovered by William Herschel in 1784 it was also observed by John Herschel.

  It is variously classified as a spiral or lenticular galaxy with NASA/IPAC Extragalactic Database (NED) suggesting a classification of SA(r)0/a which suggests an odd lenticular. The nucleus contains a mild AGN of the LINER type. The galaxy does show the remains of a bar as well as copious amounts of dust.

  NGC 7013 is thought to lie at a distance of between 37 and 41 million light-years from us. At this distance it would be perhaps 42000 light-years across.

  The GALEX image in the UV suggests there may be a ring of star formation going on around the nuclear region. Radio observations suggest there are two rings of HI gas in the galaxy with little gas in between them. The small bulge-to-disk ratio and the slow rotation velocity suggest that NGC 7013 is a low-mass, low-density galaxy unlike the more luminous, typical lenticular galaxies. The galaxy may thus be a former late-type spiral galaxy which has exhausted most of its interstellar gas, either by star formation or by internal sweeping.

  Hubble has observed this galaxy but there appears to be no colour image available only this black and white one. As the galaxy is only two degrees from the Veil nebula it suffers quite a bit of interstellar extinction. I have not been able to find any decent amateur colour images of the galaxy but there is a nice black and white one by Martin Germano. Deep amateur images such as this one by Jim Thommes show some of the dust present in the area.

  Although NGC 7013 itself is quite bright for owners of large telescopes there is a faint galaxy just of the southern edge catalogued at about 16th magnitude. It seems to be catalogued as PGC 1881063, although NED only has designations for it from the infra-red WISE and 2MASS surveys. The two galaxies are probably not associated as PGC 1881063 would appear to lie a long way in the background with distances suggested at 285 Mpc.

  NGC 7013 does not make it into any of the standard observing guides such as the The Night Sky Observer's Guide (NSOG) and Luginbuhl and Skiff (L&S). It should however be visible at a stretch in 25cm and I suspect easily visible in 35cm from the UK. It does make the Herschel 3 list, although this is mostly faint unremarkable galaxies. It does lie in a rich starfield so this may distract from the galaxy. I would suggest using a medium power when trying to find it.

  Owen Brazell - Galaxy Section Director

  And as an addition to this month's article, this is a very nice image of NGC 7013 by Denis Janky that I found on Astrobin.

• NGC 6956 in Delphinus

  July 2023 - Galaxy of the Month

  I apologise for the short GOM this month but galaxies are not easy to find from the UK in the summer. Our challenge this month is the faint galaxy NGC 6956 in Delphinus.

  Discovered by William Herschel in 1784, NGC 6956 is a barred spiral galaxy that was recently imaged by the Hubble Space Telescope (HST) as part of a program to calibrate the distance scale. The Hubble observations allowed scientists to study the Cepheid variable stars in it and they, along with the Type Ia SN 2013fa, allowed scientists to work on the distance relationships. It has also hosted 2 other supernovae in the last 10 years as well.

  NGC 6956 is thought to lie about 214 million light-years away. It is part of the isolated galaxy triplet known as KTG 71 and is also included in the galaxy group LGG 440, which includes NGC 6956 as well as UGC 11620 and UGC 11623. The galaxies appear to be physically associated but are not interacting at this time. Two of the galaxies appear to be barred spirals whilst the third is a lenticular. Perhaps unsurprisingly, apart from studies of the supernovae discovered in NGC 6956, not a great deal of work has been done on these galaxies. As these galaxies lie on the edge of the Milky Way the group suffers from quite a bit of extinction.

  The group is very close together so a high-power eyepiece maybe best to use when the group is acquired. In theory all three should be in range of a 37cm telescope but I suspect that to pick up the fainter ones is going to require a 45cm or greater from UK skies.

  The Night Sky Observer's Guide (NSOG) Vol. 2 suggest that a 16-18” telescope is required to see much of NGC 6956 but does not mention any observations of the two UGC galaxies. Steve Gottlieb does mention observations of them with his 24” at high altitude and says they are faint which suggests they are going to be out of reach of visual observers from the UK. Interestingly Luginbuhl and Skiff (L&S) suggest NGC 6956 can be seen with 25cm, although this may well have also been from high altitude. There are some observations of the group using an EAA type system. Observations in the UK made with a 40cm telescope suggest it is round and small and quite faint, although this was probably not from a good site. The group is also included in Alvin Huey’s galaxy trios booklet.

  Owen Brazell - Galaxy Section Director

• NGC 5363 in Virgo

  June 2023 - Galaxy of the Month

  Every year I wonder whether to do a GOM for the months of June and July as it no longer gets astronomically dark here at the latitude of the UK to observe anything except bright globular clusters and every year I try and keep the thread going. This month I have chosen the bright pair of galaxies NGC 5363 and NGC 5364 at the eastern end of Virgo. Perhaps as expected they were both discovered by William Herschel. NGC 5363 was found in 1784 but NGC 5364 had to wait another two years until 1786 for its discovery.

  NCG 5363 is part of the NGC 5364 group of galaxies which itself is part of the Virgo III cloud, a chain of perhaps 72 galaxy groups galaxies spread out to the east of the main Virgo group. See An Atlas of The Universe website for more information on the Virgo III cloud.

  NGC 5363 is characterised as a lenticular galaxy but it seems to contain a large amount of dust which appears to form a spiral shape along with shells of material which suggests a recent merger event. The nucleus is also an AGN of the LINER type. In contrast NGC 5364 is an almost face on grand design spiral. Hubble captured an image of its inner core. Unfortunately, John Herschel independently found this galaxy so it also sometimes goes under the name NGC 5317.

  The NGC 5364 group, also known as LGG 362, contains 7 NGC galaxies in NGC 5348, NGC 5356, NGC 5360, NGC 5364, NGC 5363, NGC 5300 and NGC 5338. The group is spread out over a degree of sky. Most of the rest of the galaxies were also found by William Herschel, although a number were also independently discovered by Bindon Stoney using the 72” at Birr. The group is thought to lie at a distance of about 65 million light-years.

  NGC 5363 and NGC 5364 form a non-interacting pair, although they may be in the early stages of a gravitational interaction. Bob Franke's website has a nice image of the pair and Thomas Henne provided a wide field view of the group in Picture of the Month.

  NGC 5363 and NGC 5364 make several lists including the Astronomical League’s (AL) H400 list and Stephen O’Meara’s Hidden Treasures list (number 72). O’Meara claims that both of these galaxies are visible in a 4” (10cm) refractor but I am guessing this is from his high mountain site.

  NGC 5363 and 5364 are pretty close together and both should fit in the same field of view using a medium power eyepiece. I suspect that only the core of NGC 5364 will be seen except with larger instruments as it is a close to face on spiral. The Night Sky Observer's Guide (NSOG) Vol. 2 suggests that NGC 5363 can be seen with 20-25cm instruments as a stellar core. Larger instruments should bring out more of the halo. NGC 5364 may require 35cm or more to see much and to find the small edge on galaxy NGC 5356 will probably require 40-45cm scopes under anything but the best conditions. I suspect that 45-50cm may be required to find the other edge on galaxy NGC 5360.

  As an aside this group is next to ACO 1809 but I suspect that is one for the imagers or EAA people, or those using very large telescopes from high sites.

  Interestingly NGC 5363 was also included as the C component of the double star BU 1438, also known as STT 273.

  Owen Brazell - Galaxy Section Director

• Arp 232 in Leo

  May 2023 - Galaxy of the Month

  As the skies start to get brighter as we approach the summer season in the northern hemisphere, I have chosen the relatively bright galaxy NGC 2911, also known as Arp 232, as my galaxy of the month. The galaxy is also included in the extended Vorontsov-Velyaminov (VV) catalogue as VV 1290.

  Lying in the constellation of Leo, NGC 2911 was discovered by William Herschel in 1784. It is catalogued as a lenticular galaxy, although unusually for that type of galaxy it does contain a number of dust lanes. Arp catalogued it as an example of his galaxies in fission group, but also suggested that it might have concentric rings. NASA/IPAC Extragalactic Database (NED) suggests it is part of WBL 226, a small group of three galaxies, which also contains NGC 2914 along with UGC 5093.

  The nucleus of NGC 2911 appears to contain an AGN of the LINER type, which suggests there maybe, or have been interactions in the group. The AGN has also been classified as a type 3 Seyfert. There does not seem to be a lot of activity in the nucleus given that NGC 2911 is practically invisible in the UV images from GALEX.

  There is also some confusion in the group as an object (PGC 27167) was found that some sources include as NGC 2912. This cannot be true as studies of the original discovery notes for NGC 2912 show it cannot be this object and the object included in the New General Catalogue of Nebulae and Clusters of Stars (NGC) as NGC 2912 is now thought to be just a star.

  It is unlikely that NGC 2911 is interacting with NGC 2914. The group lies at a distance of perhaps 155 million light-years from us. Perhaps surprisingly for an Arp object there does not seem to have been a lot of research published on it. NGC 2914 was also included by Arp in his catalogue as Arp 137 so you get two Arp objects in the same field. NGC 2914 is also classified as a lenticular galaxy but this time showing what appears to be tidal tails. It may also be an example of a polar ring galaxy.

  The whole group is very compact and all three objects will fall in the field of a high power ultra-wide field eyepiece. A medium power field will also include the galaxy NGC 2919. Some sources suggest that this galaxy may also be part of the NGC 2911 group but it is probably unlikely. The Night Sky Observer's Guide (NSOG) Vol. 2 suggests that this galaxy group maybe more challenging than I suggested and it is a target for 40-45cm scopes and even with those NGC 2914 is no more than a faint patch. UGC 5093 is suggested to be an AV object with that class of telescope. Observations form the UK with a 40cm telescope would fit those notes with NGC 2911 being described as a faint oval.

  Owen Brazell - Galaxy Section Director

• NGC 3432 in Leo Minor

  April 2023 - Galaxy of the Month

  As we move into the brighter spring skies, I have stayed in the constellation of Leo Minor for this month’s GOM.

  NGC 3432 was first discovered by William Herschel in 1785 and was included by Halton Arp in his atlas of peculiar galaxies as Arp 206. It was also added as VV11 in Vorontsov-Velyaminov’s catalogue.

  NGC 3432 appears to be a barred spiral galaxy seen edge-on and is interacting with its neighbour the dwarf galaxy UGC 5983. This interaction appears to be causing intense star formation in NGC 3432 as well as filaments between them. The GALEX satellite image in the UV shows that star formation is occurring throughout the galaxy. Due to the amount of dust the core of the galaxy is not well seen.

  Interestingly despite all the star formation going on NGC 3242 is not classified as a starburst galaxy. This maybe because the number of really massive stars being formed is not that high yet. It is suggested that the interaction with UGC 5983 took place very recently, say less than 400 million years ago and that is not enough for a full starburst to get going, in fact the star formation rate is unusually low at the moment. It appears that both ends of NGC 3432 are strongly warped from the gravitational attraction.

  The pair is thought to lie about 30 million light-years from us. NGC 3432 was home to an unusual transient event catalogued as SN 2000ch, initially catalogued as a type II supernova it was later shown to be an LBV like Eta Car as it underwent numerous brightening events.

  There is a Hubble image on NASA's website, although a more normal coloured image by the HST can be seen on NGC 3432’s Wikipedia page.

  Interestingly the interaction does not appear to have sparked that much star formation in UGC 5983. There is an odd condensation though in NGC 3432 off to its northern end. At about 55,000 light-years across NGC 3432 is a relatively small galaxy. UGC 5983 is only 12-15 thousand light-years across and as such is a dwarf galaxy, about the size of the LMC. Observations suggest that NGC 3432 may hide an AGN of the LINER type at its core.

  The galaxy makes it into a number of popular observing lists including the Astronomical Leagues H400 list and Stephen O’Meara’s The Secret Deep.

  The visibility of the galaxy seems to depend on the observer’s location and the companion galaxy UGC 5983 appears to be very difficult to spot so that is the challenge for larger telescope observers.

  The Night Sky Observer's Guide (NSOG) suggests that in 20-25cm telescopes the galaxy is visible as a long spindle, which is backed up by observations from the UK. In 40-45cm telescopes the suggestion is that it will show some of the mottling in the spindle. Unfortunately, there are no large telescope observations in NSOG. There are also observations of the galaxy with a wide range of telescopes on the Webb Deep-Sky Society Observer's Handbook (WSDSOH) Volume 4.

  I suspect that using a medium power may be best to see this galaxy, although if the seeing and transparency conditions are good then high power may tease out UGC 5983.

  Owen Brazell - Galaxy Section Director

• NGC 3395 in Leo Minor

  March 2023 - Galaxy of the Month

  This month’s challenge is the galaxy pair in Leo Minor, NGC 3395 and NGC 3396, also known as Arp 270 and VV 246. The pair were discovered by William Herschel in December 1785. They are part of the NGC 3430 group, also known as LGG 218, which lists about 15 members lying at about 30 Mpc.

  There are a number of other fainter galaxies in the field that were discovered by Stephan Javelle using a 76cm refractor, these being IC 2604, IC 2605, IC 2608 and IC 2612, although IC 2605 is just a bright spot in NGC 3395. IC 2612 is not associated with the group being a background galaxy.

  UV observations of the group with the GALEX satellite show that large amounts of star formation appear to be going on in both NGC 3395 and 3396 along with the nearby galaxy NGC 3430, in fact NGC 3395 is classified as having a starburst nucleus.

  The galaxies appear to be in the early stages of an interaction and are still separate, although at the calculated distance they would only be about 12 kpc apart, about a third of the distance between our Milky Way and the LMC. The galaxies appear to be overlapping and a bridge and tidal tails have been detected in the pair. The suggestion is that they have already had one close pass and the second will be due in 10 million years or so.

  NGC 3395 has been classified as a distorted spiral and NGC 3396 as Im (a Magellanic style irregular), although with its bright line spectrum it has also been classified as a Wolf-Rayet galaxy because of all the massive star formation going on. NGC 3395 was one of the galaxies that the Rosse team at thought to be spirals after observations using the 72” at Birr.

  Perhaps surprisingly I can’t find an HST image of the pair. One assumes because they have strong infra-red emission, probably caused by the strong star formation, that at some point the JWST will have a look.

  The NGC 3395/3396 pair is one of the best and brightest of the galaxies in the Arp atlas. NGC 3395 makes the Astronomical League’s H400 list, although the brighter of the pair, NGC 3396 does not.

  The galaxies are a close pair so using high power to separate them will work well. A medium power field judiciously placed will also include the low surface brightness galaxy NGC 3430 in the same field of view as the others. This pair should be considerably easier to see than the last two GOM’s.

  There are many reports of people seeing them with a 25cm (10”) scope which suggest both galaxies are easy to see. The Night Sky Observer's Guide Vol. 2 suggests that at a medium power in 40-45cm (16-18”) scopes the pair is well seen and looks like a butterfly. The nucleus of NGC 3395 is almost stellar. The pair have an entry in OOTW in the DSF forum.

  Owen Brazell - Galaxy Section Director

• Hickson 40 in Hydra

  February 2023 - Galaxy of the Month

  After last months really rather hard challenge we have something slightly easier this month in the galaxy group Hickson 40, also known as Arp 321 and VV 116, in Hydra.

  Although this may be challenging because of its altitude from northern climes it is a really nice tight group. Consisting of three spirals, an elliptical and a lenticular galaxy this is one of the tightest groups in the Hickson catalogue. All the galaxies appear to contain compact sources, suggested to be supermassive black holes, at their centres. The size of the group is so small that all five galaxies could fit in a volume less than twice the size of our Milky Way galaxy.

  Although such compact groupings are regularly found in large galaxy clusters Hickson 40 appears to be a rather isolated field group. There actually appear to be 7 galaxies in the group but only 5 are easily seen. The group is located perhaps 300 million light-years away and is in the process of undergoing a merger to form one large elliptical galaxy. This may take place in a billion years or so.

  Hubble imaged these galaxies as part of its 32 birthday study. The group was classified by Arp as part of his class of galaxy groups.

  This group is going to be challenging for observers as none of the galaxies are bright enough to have an NGC or IC designation and the low altitude as seen from the UK, although it does crawl above the 30 degree line, will not help either.

  The brightest galaxy of the group is MCG 1-25-9 at 13.8 B so it should be visible in 30-40cm scopes from a dark sky. The rest of the group is somewhat fainter. The group is so tight that you should try using the highest power your telescope and the conditions will allow as this is also going to be the best when trying to tease out the details of the fainter members of the group.

  Unfortunately, despite being a Hickson group it does not appear in the Night Sky Observer's Guide Vol. 2. There is some information on the group on Reiner Vogel’s Hickson page.

  Owen Brazell - Galaxy Section Director

• NGC 1740 in Orion

  January 2023 - Galaxy of the Month

  For this month’s challenge I am going very deep into Orion. I am going to throw this out there and apologise that the challenge may be too extreme. The challenge is the faint galaxy pair NGC 1740 and NGC 1753.

  NGC 1740 was discovered in 1830 by John Herschel using an 18.3 speculum metal telescope. NGC 1753 had to wait another 50 years or so for Lewis Swift to find it using a 16” refractor in 1889, I suspect at this date from the Lowe observatory on Echo Mountain. Unfortunately it seems that confusion arose in the area and it appears that there is some conflict between the NGC numbers 1740 and 1742 due to an error in John Herschel’s positions. NGC 1742 is almost certainly just a star. It was found by Ball using Lord Rosse’s 72” at Birr.

  NGC 1740 is classified as a lenticular galaxy S0 at a distance of perhaps 59 Mpc. NGC 1753 is classified as a spiral SBa (pec) with a redshift derived distance of 57 Mpc so they may be a physical pair. Perhaps unsurpingly for such non-descript galaxies there is not much written on them. Both galaxies do appear surprisingly bright in the GALEX images which suggests that there is some star formation going on, which would be surprising for a lenticular galaxy as most of the star forming gas is normally stripped out of these.

  Holmberg thought NGC 1740 was a double nebula with NGC 1742 and classified it as Holmberg 84 in his catalogue of double and multiple galaxies. Unfortunately, as noted above NGC 1742 does not exist. It is possible that Barrachi using the 40” Great Melbourne telescope found these two galaxies independently.

  I have to say both of these are going to be very challenging objects and probably a bit faint really for any spectacular views. The altitude is also not going to help as seen from the UK but they do rise above 30 degrees. The galaxies are relatively close together and will be in the field of view of a modern widefield eye at a power of 265x. I suspect that using a high power to increase the contrast is probably going to be the only way to pick up NGC 1753. Using a medium power eyepiece may also bring the galaxy NGC 1729 into the field. This is also a faint object though.

  Steve Gottlieb suggests that even with his old 17.5” both these galaxies were no more than faint smudges. Perhaps unsurprisingly they are not in the Night Sky Observer's Guide (NSOG) Vol. 1.

  Owen Brazell - Galaxy Section Director