IC 883

Interacting Galaxy IC 883

Observation data (J2000.0 epoch)
Constellation| Canes Venatici[1]
Right ascension|  13h 20m 35,5s [2]
Declination| +34° 8′ 19″ [2]
Redshift| 6954 ± 16 km/s[3]
Distance| 320.9 Mly (98.4 Mpc)[2]
Apparent magnitude (V)| 13.8[2]
Characteristics
Type| Irr (Im/P) [2]
Apparent size (V)| 2′.4 × 0′.7[3]
Notable features| Interacting galaxies
Other designations
Arp 193 • UGC 8387 • PRC D-25 • IRAS 13183+3423 • PGC 46560 • VV 821 • ZWG 189.54 • 1ZW 56 • CGCG 189-54[2][3]

IC 883 (also known as Arp 193, IRAS 13183+3423, PGC 46560 and UGC 8387) is an irregular galaxy that is about 321 million light years away from Earth. It is located in the constellation Canes Venatici. Its largest radius is 1.4 (131 thousand light years), and smallest 0.7 angular minutes (65 thousand light years).[b] It was discovered by Rudolf Ferdinand Spitaler on May 1 1891.[2][4][5]

IC 883 is classified a luminous infrared galaxy (LIRG).[6][7] It is a recent merger given that the galaxy has one single nucleus and two tidal tails. The molecular gas measured in IC 883 is estimated 4 billion MΘ.[8] It is known to show a radio jet originating from its nucleus travelling at a subluminal motion of 0.6-1 c.[9]

## Contents

* 1 Supernovae
* 2 References
* 3 Literature
* 4 External links

## Supernovae

Two supernovae have been observed in IC 883:

* SN 2010cu (Type II, mag. 17.7) was discovered by S. Mattila and E. Kankare on 24 February 2010.[10][11]
* SN 2011hi (Type II, mag. 17.9) was discovered by E. Kankare, S. Ryder, and S. Mattila on 11 February 2011.[12][13]

When observed in near-infrared or optical wavelengths, they are the nearest supernovae found to the nucleus of an LIRG.[14]

## References

1. ↑ seds.org
2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Entdeckung und Katalogisierung von Nebeln und Sternhaufen. "Wolfgang Steinicke-ov revizirani NGC i IC katalog". http://www.klima-luft.de/steinicke/ngcic/ngcic_e.htm.
3. ↑ 3.0 3.1 3.2 Rezultati za IC 883. "NASA/IPAC Extragalactic Database". http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=IC+883&img_stamp=yes&extend=no.
4. ↑ NGC/IC observers, Feb 21. 2016]
5. ↑ Young, C., Sid. Mess. II, 252 (1883-84).
6. ↑ Romero-Cañizales, C.; Pérez-Torres, M. A.; Alberdi, A.; Argo, M. K.; Beswick, R. J.; Kankare, E.; Batejat, F.; Efstathiou, A. et al. (2012-07-01). "e-MERLIN and VLBI observations of the luminous infrared galaxy IC 883: a nuclear starburst and an AGN candidate revealed" (in en). Astronomy & Astrophysics 543: A72. doi:10.1051/0004-6361/201218816. ISSN 0004-6361. Bibcode: 2012A&A...543A..72R. https://www.aanda.org/articles/aa/abs/2012/07/aa18816-12/aa18816-12.html.
7. ↑ Modica, F.; Vavilkin, T.; Evans, A. S.; Kim, D. C.; Mazzarella, J. M.; Iwasawa, K.; Petric, A.; Howell, J. H. et al. (2011-11-14). "Multi-Wavelength Goals Observations of Star Formation and Active Galactic Nucleus Activity in the Luminous Infrared Galaxy Ic 883" (in en). The Astronomical Journal 143: 16. doi:10.1088/0004-6256/143/1/16.
8. ↑ Modica, F.; Vavilkin, T.; Evans, A. S.; Kim, D.-C.; Mazzarella, J. M.; Iwasawa, K.; Petric, A.; Howell, J. H. et al. (2011-12-09). "Multi-Wavelength Goals Observations of Star Formation and Active Galactic Nucleus Activity in the Luminous Infrared Galaxy Ic 883". The Astronomical Journal 143 (1): 16. doi:10.1088/0004-6256/143/1/16. ISSN 0004-6256.
9. ↑ Romero-Cañizales, C.; Alberdi, A.; Ricci, C.; Arévalo, P.; Pérez-Torres, M. Á.; Conway, J. E.; Beswick, R. J.; Bondi, M. et al. (2017-01-27). "Unveiling the AGN in IC 883: discovery of a parsec-scale radio jet". Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stx224. ISSN 0035-8711.
10. ↑ Kankare, E.; Mattila, S.; Ryder, S.; Perez-Torres, M. A.; Romero-Canizales, C.; Alberdi, A.; Alonso-Herrero, A.; Colina, L. et al. (2010). "Possible Supernova in IC 883: PSN K1002-1". Central Bureau Electronic Telegrams (2213): 1. Bibcode: 2010CBET.2213....1K. http://www.cbat.eps.harvard.edu/iau/cbet/002200/CBET002213.txt.
11. ↑ "SN 2010cu". IAU. https://www.wis-tns.org/object/2010cu.
12. ↑ Kankare, E.; Ryder, S. D.; Mattila, S.; Romero-Canizales, C.; Perez-Torres, M.-A.; Alberdi, A. (2011). "Supernova 2011hi in IC 883 = PSN J13203538+3408222". Central Bureau Electronic Telegrams (2889): 1. Bibcode: 2011CBET.2889....1K. http://www.cbat.eps.harvard.edu/iau/cbet/002800/CBET002889.txt.
13. ↑ "SN 2011hi". IAU. https://www.wis-tns.org/object/2011hi.
14. ↑ Kankare, E.; Mattila, S.; Ryder, S.; Vaisanen, P.; Alberdi, A.; Alonso-Herrero, A.; Colina, L.; Efstathiou, A. et al. (2011-12-04). "Discovery of Two Supernovae in the Nuclear Regions of the Luminous Infrared Galaxy Ic 883" (in en). The Astrophysical Journal 744 (2): L19. doi:10.1088/2041-8205/744/2/L19.

## Literature

* Steinicke, Wolfgang (2007), Jakiel, Richard, ed., Galaxies and How to Observe Them, Springer, ISBN 978-1-85233-752-0, https://archive.org/details/galaxieshowtoobs0000stei
* R. J. Buta; H. G. Corwin, Jr.; S. C. Odewahn (2007). The de Vaucouleurs Atlas of Galaxies. Cambridge: Cambridge University. ISBN 978-0-521-82048-6.
* Sinnott, R. W. (1988). NGC 2000.0: The Complete New General Catalogue and Index Catalogues of Nebulae and Star Clusters. Sky Publishing. ISBN 978-0-933346-51-2.

## External links

| Wikimedia Commons has media related to Canes Venatici.

|

* NASA Astronomy Picture of the Day: When Mice Collide (12 June 2004)
* The Mice Galaxies
* Photographic Catalogue of Deep Sky Objects in Canes Venatici

Coordinates:  12h 46m 10.1s, +30° 43′ 55″

* v
* t
* e

Canes Venatici constellation

Stars (list)|

| Bayer|

* α (Cor Caroli)
* β (Chara)

|

Flamsteed|

* 2
* 3
* 4
* 5
* 6
* 7
* 9
* 10
* 11
* 14
* 15
* 16
* 17
* 18
* 19
* 20
* 21
* 23
* 24
* 25

Variable|

* R
* V
* W
* Y (La Superba)
* Z
* RS
* ST
* TT
* TU
* TX
* UX
* UZ
* VZ
* AM
* AW
* AX
* BH
* BI
* BL
* BM
* CL
* DD
* DG
* DT

HR|

* 4783
* 4784
* 4843
* 4904
* 4919
* 4945
* 4964
* 4997
* 5022
* 5025
* 5045
* 5067
* 5077
* 5083
* 5096
* 5108
* 5143
* 5145
* 5160
* 5161
* 5179
* 5180
* 5186
* 5195
* 5204
* 5215
* 5229
* 5245
* 5271

HD|

* 107610
* 109995
* 111572
* 114975
* 115444
* 121197

Gliese|

* Gliese 490
* Gliese 521
* GJ 3789
* GJ 3801

Other|

* GD 154
* HAT-P-12
* HAT-P-36

Star clusters|

| Globular|

* Messier 3

|

Galaxies|

| Messier|

* 51 (Whirlpool Galaxy)
* 63
* 94
* 106

|

NGC|

* 4109
* 4111
* 4117
* 4118
* 4135
* 4137
* 4138
* 4143
* 4145
* 4145A
* 4148
* 4151
* 4156
* 4163
* 4183
* 4187
* 4187B
* 4187C
* 4190
* 4214
* 4217
* 4218
* 4220
* 4226
* 4227
* 4229
* 4231
* 4232
* 4242
* 4244
* 4248
* 4288
* 4288A
* 4346
* 4369
* 4381
* 4389
* 4392
* 4395
* 4399
* 4400
* 4401
* 4449
* 4460
* 4485
* 4490
* 4509
* 4534
* 4542
* 4583
* 4617
* 4618
* 4619
* 4625
* 4627
* 4631
* 4655
* 4656
* 4657
* 4662
* 4687
* 4704
* 4707
* 4711
* 4719
* 4737
* 4741
* 4774
* 4800
* 4834
* 4837
* 4846
* 4861
* 4868
* 4870
* 4893
* 4901
* 4914
* 4917
* 4932
* 4938
* 4956
* 4959
* 4963
* 4985
* 4986
* 4987
* 4998
* 5002
* 5003
* 5005
* 5009
* 5014
* 5021
* 5023
* 5025
* 5029
* 5033
* 5040
* 5074
* 5083
* 5093
* 5096
* 5098A
* 5098B
* 5103
* 5107
* 5112
* 5117
* 5123
* 5127
* 5131
* 5141
* 5142
* 5143
* 5145
* 5149
* 5154
* 5157
* 5166
* 5166B
* 5169
* 5173
* 5187
* 5195
* 5198
* 5199
* 5214
* 5214A
* 5223
* 5225
* 5228
* 5229
* 5233
* 5238
* 5240
* 5243
* 5259
* 5263
* 5265
* 5267
* 5271
* 5273
* 5274
* 5275
* 5276
* 5277
* 5280
* 5282
* 5287
* 5289
* 5290
* 5296
* 5297
* 5301
* 5303
* 5303B
* 5305
* 5311
* 5312
* 5313
* 5318
* 5319
* 5320
* 5321
* 5325
* 5325B
* 5326
* 5336
* 5337
* 5341
* 5346
* 5347
* 5349
* 5350
* 5351
* 5352
* 5353
* 5354
* 5355
* 5358
* 5361
* 5362
* 5371
* 5377
* 5378
* 5380
* 5383
* 5396
* 5399
* 5401
* 5403
* 5406
* 5407
* 5410
* 5421A
* 5421B
* 5433
* 5439
* 5440
* 5441
* 5444
* 5445

Other|

* B2 1225+317
* 3C 268.4
* 3C 270.1
* 3C 280
* 3C 280.1
* 3C 285
* 3C 286
* 3C 288
* 3C 293
* 3C 294
* Canes Venatici I
* Canes Venatici II
* DDO 125
* DDO 169
* IC 883
* IC 4182
* KPG 404 (NGC 5394/5395)
* Markarian 59
* UGCA 292
* I Zw 36

Galaxy
clusters|

* Abell 1758
* Abell 1763
* Canes II Group
* CL J1226+3332
* M51 Group
* M94 Group
* NGC 4631 Group

Other|

* Giant Void
* GRB 060206
* SN 1937C
* SN 1985F
* SN 1994I
* SN 2005cs
* SN 2008ax

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