Object name: ARP320

Designation(s): ARP320, NGC3746, NGC3745, NGC3748, NGC3750, NGC3751, NGC3753, NGC3754, PGC036010,

Arp 320/Copeland\'s Septet is a group of 7 galaxies though you\'ll see 9 main galaxies in the center of the field. A finder chart of the 7 that are members of the \"official\" septet http://www.ngcicproject.org/dss/n/3/n3753.jpg
Note the blob above the label for NGC 3754 is a plate defect so you won\'t see it in my image. It is also known as Hickson 57. The main galaxy in the group is NGC 3753 also known as ARP 320. The reason for so many names is just that each astronomer has some reason to study it and puts it in their catalog. Before long there are a ton of catalog entries for the same thing. Besides NGC 3753 is also known as: UGC 06602, VV282a, KUG1135+222, CGCG127-012S, CGCG1135.4+2216, MCG+04-28-010, PGC03616, UZC J113753.8+215852 and [BDG09] J113753.9+215853 to name a few. The group is also known as Copeland\'s septet, HCG 057, WBL 343-005, USGC U404 and UZC-CG 142, RSCG 43 and others. Confused yet?

The group is about 410 to 440 million light years distant and somewhat red. I suspect this is due to lots of dust between us and the group though one galaxy does show some blue color. But two of the redder galaxies have \"retired\" nuclei. This means star formation has virtually ceased though some emission lines of LINER galaxies are still seen. This usually is interpreted to mean they are about to become red and dead galaxies. Several papers mention this color problem but none I saw gives an answer or even a guess as to why the group but for NGC 3754 is so red. Some of it was discovered by Ralph Copeland on February 9, 1874 (NGC 3746, 3750 and 3753) and the rest on April 5, 1874 (NGC 3745, 3748, 3751 and 3754). He got their position rather wrong by about 1.5 minutes of Right Ascension and about 15 arcmin of NPD. Enough that my field would have missed it using Copeland\'s position. But since no other group is in the area and its description fits his identification is certain. As to why 4 were found in April and 3 in February, I couldn\'t discover.

Just under NGC 3748 is PGC 36010 an S0/a galaxy that some consider part of Arp 320 but Copeland didn\'t see so it is not Copland\'s Octet. It is part of HCG 57 however. Look around the annotated image and you will see quite a few other galaxies, mostly dwarfs compared to the seven in the septet, also at the 410 to 440 million light-year distance indicating this is quite a large group.

It is quite obvious NGC 3753 is interacting with NGC 3750 by the huge plumes it has. I suppose the vertical one off the west end may be coming from NGC 3750. NGC 3753\'s southeastern plume almost looks like it is sticking its tongue out. Its dust lane is quite disturbed. Often a sign it ate something recently. While SLOAN shows a point source object just northwest of its upper end it doesn\'t show any entry for the plume. I thought it might be some low surface brightness dwarf that just happened to line up with NGC 3753 but apparently, it is just a plume. Assuming it is a plume and including the northwestern plume, I measure the full size at 300,000 light-years. Measuring just the bright disk I get 110,000 light-years.

NGC 3748 shows plumes as well indicating it did interact with one of the galaxies in the group but which one? Including plumes, it is 162,000 light-years across. The disk is much smaller at 55,000 light-years. NGC 3746 I measure at 135,000 light-years in size. I measure NGC 3750 at 140,000 light-years, NGC 3751 at 145,000 light-years and NGC 3745 at 90,000 light-years including the faint plume, mainly to the east. Omitting the plume I get 40,000 light-years making it the smallest of the 7.

The asteroid to the lower left (southeast) is (30376) 2000 JE65 at magnitude 17.7.

Arp\'s image: http://ned.ipac.caltech.edu/level5/Arp/Figures/big_arp320.jpeg

14\" LX200R @ f/10, L=4x10\' RGB=2x10\'x3, STL-11000XM, Paramount ME

Alternate Designation(s): 2MASS J11374363+2200353, 2MASS J11374445+2201167, 2MASS J11374907+2201343, 2MASS J11375051+2200451, 2MASS J11375165+2158272, 2MASS J11375380+2158520, 2MASS J11375387+2156113, 2MASS J11375492+2159080, 2MASX J11374364+2200349, 2MASX J11374443+2201170, 2MASX J11374903+2201340, 2MASX J11375047+2200450, 2MASX J11375378+2158520, 2MASX J11375386+2156110, 2MASXi J1137536+215850, 2MASXi J1137538+215611, 2MASXi J1137549+215908, 2XMM J113749.0+220133, 2XMM J113751.6+215827, 2XMM J113753.8+215849, 2XMM J113755.0+215908, ARP 320, ARP 320 NED01, ARP 320 NED02, ARP 320 NED03, ARP 320 NED04, ARP 320 NED05, ARP 320 NED06, ARP 320 NED07, ARP320, ASK 628328.0, ASK 628329.0, ASK 628330.0, ASK 628331.0, ASK 628333.0, CGCG 1135.1+2217, CGCG 1135.2+2218, CGCG 1135.3+2215, CGCG 1135.4+2216 NED01, CGCG 1135.4+2216 NED02, CGCG 127-006, CGCG 127-007, CGCG 127-009, CGCG 127-012 NED01, CGCG 127-012 NED02, CGCG 127-012N, CGCG 127-012S, Copeland Septet, Copeland Septet NED01, Copeland Septet NED02, Copeland Septet NED03, Copeland Septet NED04, Copeland Septet NED05, Copeland Septet NED06, Copeland Septet NED07, GALEXASC J113743.64+220035.9 , GALEXASC J113744.51+220118.9 , GALEXASC J113749.23+220133.5 , GALEXASC J113750.61+220045.3 , GALEXASC J113751.62+215826.3 , GALEXASC J113753.69+215612.9 , HCG 057, HCG 057A, HCG 057B, HCG 057C, HCG 057D, HCG 057E, HCG 057F, HCG 057G, HCG 057H, HDCE 0661 NED002, HDCE 0661 NED004, IRAS 11352+2216, IRAS F11352+2215, KUG 1135+222, LDCE 0826 NED002, LDCE 0826 NED004, MAPS-NGP O_376_2858137, MAPS-NGP O_376_2858854, MAPS-NGP O_376_2859071, MAPS-NGP O_376_2859431, MCG +04-28-004, MCG +04-28-005, MCG +04-28-007, MCG +04-28-008, MCG +04-28-009, MCG +04-28-010, MCG +04-28-011, NGC 3745, NGC 3746, NGC 3748, NGC 3750, NGC 3751, NGC 3753, NGC 3754, NGC3745, NGC3746, NGC3748, NGC3750, NGC3751, NGC3753, NGC3754, NPM1G +22.0340, NSA 112840, NSA 112841, NSA 112842, NSA 112843, NSA 112845, NSA 139936, NSA 139941, NSA 139944, NVSS J113754+215910, PCC N79-278, PGC 035997, PGC 036001, PGC 036007, PGC 036010, PGC 036011, PGC 036016, PGC 036017, PGC 036018, PGC036010, RSCG 43, SDSS J113743.62+220035.3, SDSS J113744.43+220116.5, SDSS J113744.43+220116.6, SDSS J113749.06+220134.1, SDSS J113750.49+220045.0, SDSS J113750.49+220045.1, SDSS J113751.63+215827.1, SDSS J113751.63+215827.2, SDSS J113753.79+215852.3, SDSS J113753.85+215611.3, SDSS J113754.91+215907.8, SDSS J113754.92+215907.7, SDSS J113754.92+215907.8, SPRC 203, SSTSL2 J113744.44+220116.6, SSTSL2 J113749.06+220134.2, SSTSL2 J113750.50+220045.2, SSTSL2 J113751.66+215827.3, SSTSL2 J113753.80+215851.4, SSTSL2 J113753.87+215611.2, SSTSL2 J113754.92+215908.0, UGC 06597, UGC 06601, UGC 06602, UGC 06602 NOTES01, UGC 06602 NOTES02, UGC 06602 NOTES03, USGC U404 NED01, USGC U404 NED02, USGC U404 NED04, USGC U404 NED05, USGC U404 NED06, UZC J113743.6+220035, UZC J113749.1+220134, UZC J113751.7+215827, UZC J113753.8+215852, UZC J113754.9+215908, UZC-CG 142 NED01, UZC-CG 142 NED02, UZC-CG 142 NED03, UZC-CG 142 NED04, VV 282a, VV 282b, VV 282c, WBL 343, WBL 343-001, WBL 343-002, WBL 343-003, WBL 343-005, X-CLASS 1937, [BDG98] J113743.6+220034, [BDG98] J113744.5+220116, [BDG98] J113749.1+220133, [BDG98] J113750.5+220045, [BDG98] J113751.7+215826, [BDG98] J113753.9+215610, [BDG98] J113753.9+215853, [BDG98] J113755.0+215908, [DZ2015] 666-01, [DZ2015] 666-02, [DZ2015] 666-04, [DZ2015] 667-01, [DZ2015] 667-03, [RLA2016] J174.4652+21.9742, [RPG97] 145, [TTL2012] 139607, [TTL2012] 139608, [TTL2012] 139609, [TTL2012] 139610, [TTL2012] 139612, [ZGH93] G021,