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292:. Additionally, the galaxy is depicted having a ring-like appearance. The most likely scenario for this appearance in PGC 32620, is that the elliptical galaxy penetrated through its disk, causing it to become semi-annular with a large single
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protruding out. This spiral arm in turn, then branches out in a form of a tidal arm, where
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554:"The effects of interactions on spiral galaxies. I. Nuclear activity and star formation"
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552:
Keel, W. C.; Kennicutt, R. C., Jr.; Hummel, E.; van der Hulst, J. M. (1985-05-01).
480:"ULTRAVIOLET/OPTICAL/INFRARED COLOR SEQUENCES ALONG THE TIDAL RING/ARM OF Arp 107"
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Arp 107 is made of two separate galaxies. The larger galaxy to the left is
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456:. Spitzer Science Center, California Institute of Technology. 9 June 2005
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623:"UV/Optical/IR Color Sequences Along the Tidal Ring/Arm of Arp 107"
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Lapham, Ryen C.; Smith, Beverly J.; Struck, Curtis (2013-03-13).
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Lapham, Ryen C.; Smith, Beverly J.; Struck, Curtis (2013-03-28).
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529:"Hubble Captures Stunning Collision of Two Galaxies | Sci.News"
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Data
Release 2: Summary of the contents and survey properties"
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image). These galaxies are different in which one is a
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355:; et al. (Gaia collaboration) (August 2018).
16:Interacting galaxy in the constellation Leo Minor
1289:
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430:Centre de données astronomiques de Strasbourg
249:are in the process of colliding and merging.
8:
311:False-color infrared image of Arp 107, from
87:+30° 03′ 28.3630″
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33:Arp 107 photograph taken using NASA/ESA
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1268:. You can help Knowledge (XXG) by
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14:
1264:This galaxy-related article is a
450:"Interacting Galaxy Pair Arp 107"
288:and it is classified as a type 2
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1234:
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527:Lazaro, Enrico de (2023-09-18).
277:being connected by a bridge and
533:Sci.News: Breaking Science News
454:Spitzer Space Telescope website
717:Leo Minor in Chinese astronomy
1:
665:: VV 233 -- Seyfert 2 Galaxy
366:Astronomy & Astrophysics
284:The nucleus of PGC 32620 is
103:Heliocentric radial velocity
506:10.1088/0004-6256/145/5/130
400:10.1051/0004-6361/201833051
39:Advanced Camera for Surveys
1351:
1251:
712:List of stars in Leo Minor
701:Constellation of Leo Minor
273:while the other one is an
223:(designated separately as
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219:is a pair of interacting
200:
26:
558:The Astronomical Journal
484:The Astronomical Journal
598:"A peculiar proceeding"
390:2018A&A...616A...1G
313:Spitzer Space Telescope
281:made of dust and gas.
315:
300:of both old and young
265:, (as depicted in the
35:Hubble Space Telescope
310:
1315:Interacting galaxies
658:at Wikimedia Commons
298:star-forming regions
190:interacting galaxies
181:1.40' × 0.11' ?
163:(PGC 32620), 70,000
316:
196:Other designations
128:Apparent magnitude
46:Observation data (
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654:Media related to
602:www.esahubble.org
325:Antennae Galaxies
275:elliptical galaxy
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302:star populations
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186:Notable features
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253:Characteristics
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644:External links
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290:Seyfert galaxy
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205:5984, VV 233,
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271:spiral galaxy
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240:constellation
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229:MCG+05-26-025
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173:Apparent size
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151:SA(s)cP / E1P
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59:Constellation
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20:
1335:Galaxy stubs
1270:expanding it
1263:
1248:
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662:
630:. Retrieved
626:
616:
605:. Retrieved
601:
561:
557:
547:
536:. Retrieved
532:
522:
487:
483:
458:. Retrieved
453:
444:
433:. Retrieved
423:
370:
364:
358:
304:are present.
283:
262:
258:
256:
238:away in the
228:
224:
216:
215:
1330:UGC objects
1325:Arp objects
564:: 708–730.
236:light-years
233:450 million
209:32620/32628
167:(PGC 32628)
118:450 million
83:Declination
1309:Categories
1210:AGC 198691
1088:HD 87883 b
1080:Exoplanets
632:2024-08-16
607:2024-08-16
538:2024-08-16
490:(5): 130.
460:19 October
435:2020-05-16
380:1804.09365
336:References
294:spiral arm
279:tidal tail
107:10167 km/s
1320:Leo Minor
754:Flamsteed
627:arXiv.org
578:0004-6256
514:1538-3881
497:1303.3312
420:"Arp 107"
263:PGC 32628
259:PGC 32620
243:Leo Minor
64:Leo Minor
1240:Category
1102:Galaxies
1062:NGC 3382
952:Variable
319:See also
247:galaxies
225:UGC 5984
221:galaxies
159:348,000
113:Distance
93:Redshift
1220:IC 2497
1215:Arp 107
656:Arp 107
385:Bibcode
330:Arp 299
245:. The
217:Arp 107
97:0.03451
48:J2000.0
22:Arp 107
1205:3C 236
1200:3C 223
663:SIMBAD
576:
512:
425:SIMBAD
373:. A1.
286:active
267:Hubble
175:
130:
1193:Other
1055:Other
1046:93521
1041:87883
736:Bayer
727:Stars
492:arXiv
375:arXiv
51:epoch
1266:stub
1184:3504
1179:3486
1174:3432
1169:3430
1164:3414
1159:3396
1154:3395
1149:3344
1144:3294
1139:3254
1134:3245
1129:3021
1124:3003
1119:2859
1018:3993
1013:3979
574:ISSN
510:ISSN
462:2012
359:Gaia
227:and
156:Size
147:Type
136:14.6
1111:NGC
566:doi
502:doi
488:145
395:doi
371:616
207:PGC
203:UGC
177:(V)
132:(B)
37:’s
1311::
1028:HD
1005:HR
995:AS
990:YZ
985:VW
980:SX
975:RZ
970:RY
965:RW
942:51
937:50
932:48
922:45
917:44
912:43
907:42
902:41
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586:^
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562:90
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470:^
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344:^
165:ly
161:ly
121:ly
1297:e
1290:t
1283:v
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960:R
772:9
767:8
762:7
744:β
693:e
686:t
679:v
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568::
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504::
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403:.
397::
387::
377::
357:"
53:)
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
