NGC 5135
| NGC 5135 | |
|---|---|
 NGC 5135 by legacy surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Hydra |
| Right ascension | 13h 25m 44.1s[1] |
| Declination | −29° 50′ 01″[1] |
| Redshift | 0.013693 ± 0.000020 [1] |
| Heliocentric radial velocity | 4,105 ± 6 km/s[1] |
| Distance | 194 Mly[1] |
| Apparent magnitude (V) | 12.9 |
| Characteristics | |
| Type | SB(l)ab [1] |
| Apparent size (V) | 2.6′ × 1.8′[1] |
| Notable features | Seyfert galaxy |
| Other designations | |
| ESO 444-G032, MCG -05-32-013, PGC 46974[1] | |
NGC 5135 is a barred spiral galaxy located in the constellation Hydra. It is located at a distance of about 200 million light years from Earth. It was discovered by John Herschel on May 8, 1834.[2] It is a Seyfert galaxy.[1]
Characteristics
NGC 5135 has well defined spiral arms and is considered a grand design spiral galaxy. There is star formation along the leading edges of the arms.[3] There are dust lanes along the bar that curve towards the centre of galaxy.[4] Spiral arms become less well structured in the central regions.[3]
NGC 5135 is a bright source in infrared light and with total infrared luminosity of 1011.16−1011.23 L☉ is considered a luminous infrared galaxy.[5][6] Also strong ultraviolet emission was detected in the central 2 arcseconds of the galaxy, with a dozen of prominent knots, indicative of a recent starburst.[7] The total star formation rate in the galaxy is estimated to be 15.61 ± 1.87 M☉ per year.[6] Knots of gas measuring 45–180 parsecs across are detected along the inner spiral arms in CO(6-5) imaging and some of them are associated with starburst regions.[8]
The nucleus of NGC 5135 has been found to be active and it has been categorised as a type II Seyfert galaxy.[9] The most accepted theory for the energy source of active galactic nuclei is the presence of an accretion disk around a supermassive black hole. The mass of the black hole in the centre of NGC 5135 is estimated to be 107.29 (19 million) M☉.[10]
The active nucleus is obscured in X-rays by Compton-thick material with a column density of 6.7+16.6
−2.8×1024/cm2.[11] An ionization cone has been detected in [Si vi] emission that extends for 600 parsec from the nucleus. To the ionization of the gas apart from the active nucleus also contribute supernova remnant shocks and young stars.[12]
One supernova has been observed in NGC 5135: SN 2023dpj (type II, mag. 17).[13]
Nearby galaxies
NGC 5135 belongs to a galaxy group known as LGG 351 or NGC 5135 group. Other members of the group include ESO 444- 12, NGC 5124, IC 4248, NGC 5150, NGC 5152, NGC 5153, IC 4275, NGC 5182, ESO 444- 47, ESO 444- 15, ESO 444- 21 and IC 4251,[14] along with NGC 5126. IC 4248, which lies 13.5 arcminutes from NGC 5135 and form a pair,[15] looks distorted and asymmetrical.[16]
See also
References
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 5135. Retrieved 2023-05-06.
- ^ Seligman, Courtney. "NGC 5135". Celestial Atlas. Retrieved 19 November 2018.
- ^ a b Martini, Paul; Regan, Michael W.; Mulchaey, John S.; Pogge, Richard W. (June 2003). "Circumnuclear Dust in Nearby Active and Inactive Galaxies. I. Data". The Astrophysical Journal Supplement Series. 146 (2): 353–406. arXiv:astro-ph/0212396. Bibcode:2003ApJS..146..353M. doi:10.1086/367817.
- ^ Sandage, A., Bedke, J. (1994), The Carnegie Atlas of Galaxies. Volume I, Carnegie Institution of Washington
- ^ Sanders, D. B.; Mazzarella, J. M.; Kim, D.-C.; Surace, J. A.; Soifer, B. T. (October 2003). "The IRAS Revised Bright Galaxy Sample". The Astronomical Journal. 126 (4): 1607–1664. arXiv:astro-ph/0306263. Bibcode:2003AJ....126.1607S. doi:10.1086/376841. S2CID 14825701.
- ^ a b Gruppioni, C.; Berta, S.; Spinoglio, L.; Pereira-Santaella, M.; Pozzi, F.; Andreani, P.; Bonato, M.; De Zotti, G.; Malkan, M.; Negrello, M.; Vallini, L.; Vignali, C. (1 June 2016). "Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high- z Universe". Monthly Notices of the Royal Astronomical Society. 458 (4): 4297–4320. arXiv:1603.02818. doi:10.1093/mnras/stw577.
- ^ Gonzalez Delgado, Rosa M.; Heckman, Timothy; Leitherer, Claus; Meurer, Gerhardt; Krolik, Julian; Wilson, Andrew S.; Kinney, Anne; Koratkar, Anuradha (20 September 1998). "Ultraviolet-Optical Observations of the Seyfert 2 Galaxies NGC 7130, NGC 5135, and IC 3639: Implications for the Starburst–Active Galactic Nucleus Connection". The Astrophysical Journal. 505 (1): 174–198. arXiv:astro-ph/9806107. Bibcode:1998ApJ...505..174G. doi:10.1086/306154. S2CID 119098033.
- ^ Cao, Tianwen; Lu, Nanyao; Xu, C. Kevin; Zhao, Yinghe; Kalari, Venu Madhav; Gao, Yu; Charmandaris, Vassilis; Santos, Tanio Diaz; Werf, Paul van der; Cao, Chen; Wu, Hong; Inami, Hanae; Evans, Aaron (18 October 2018). "ALMA Observation of NGC 5135: The Circumnuclear CO (6–5) and Dust Continuum Emission at 45 pc Resolution". The Astrophysical Journal. 866 (2): 117. arXiv:1809.06283. Bibcode:2018ApJ...866..117C. doi:10.3847/1538-4357/aae1f4.
- ^ Levenson, N. A.; Weaver, K. A.; Heckman, T. M.; Awaki, H.; Terashima, Y. (10 February 2004). "Accretion and Outflow in the Active Galactic Nucleus and Starburst of NGC 5135". The Astrophysical Journal. 602 (1): 135–147. arXiv:astro-ph/0310669. Bibcode:2004ApJ...602..135L. doi:10.1086/380836. S2CID 16284435.
- ^ Marinucci, Andrea; Bianchi, Stefano; Nicastro, Fabrizio; Matt, Giorgio; Goulding, Andy D. (1 April 2012). "The Link Between the Hidden Broad Line Region and the Accretion Rate in Seyfert 2 Galaxies". The Astrophysical Journal. 748 (2): 130. arXiv:1201.5397. Bibcode:2012ApJ...748..130M. doi:10.1088/0004-637X/748/2/130. S2CID 38183296.
- ^ Yamada, Satoshi; Ueda, Yoshihiro; Tanimoto, Atsushi; Oda, Saeko; Imanishi, Masatoshi; Toba, Yoshiki; Ricci, Claudio (7 July 2020). "Nature of Compton-thick Active Galactic Nuclei in "Nonmerging" Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-Ray Spectroscopy". The Astrophysical Journal. 897 (1): 107. arXiv:2005.08718. Bibcode:2020ApJ...897..107Y. doi:10.3847/1538-4357/ab94b1.
- ^ Bedregal, Alejandro G.; Colina, Luis; Alonso-Herrero, Almudena; Arribas, Santiago (20 June 2009). "Near-Ir Integral Field Spectroscopy Study of the Star Formation and Agn of the Lirg NGC 5135". The Astrophysical Journal. 698 (2): 1852–1871. arXiv:0904.3324. Bibcode:2009ApJ...698.1852B. doi:10.1088/0004-637X/698/2/1852. S2CID 15278691.
- ^ Transient Name Server entry for SN 2023dpj. Retrieved 25 October 2023.
- ^ Garcia, A. M. (1 July 1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
- ^ de Vaucouleurs, G.; de Vaucouleurs, A.; Corwin, J. R. (1 January 1976). "Second reference catalogue of bright galaxies". Second Reference Catalogue of Bright Galaxies. 1976. Bibcode:1976RC2...C......0D.
- ^ For, B-Q; Staveley-Smith, L; Westmeier, T; Whiting, M; Oh, S-H; Koribalski, B; Wang, J; Wong, O I; Bekiaris, G; Cortese, L; Elagali, A; Kleiner, D; Lee-Waddell, K; Madrid, J P; Popping, A; Rhee, J; Reynolds, T N; Collier, J D; Phillips, C J; Voronkov, M A; Müller, O; Jerjen, H (11 November 2019). "WALLABY early science − V. ASKAP H i imaging of the Lyon Group of Galaxies 351". Monthly Notices of the Royal Astronomical Society. 489 (4): 5723–5741. doi:10.1093/mnras/stz2501. hdl:1885/266365.
External links
Wikimedia Commons has media related to NGC 5135.
- NGC 5135 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- NGC 5135 on SIMBAD
- v
- t
- e
New General Catalogue 5000 to 5499
- 5000
- 5001
- 5002
- 5003
- 5004
- 5005
- 5006
- 5007
- 5008
- 5009
- 5010
- 5011
- 5012
- 5013
- 5014
- 5015
- 5016
- 5017
- 5018
- 5019
- 5020
- 5021
- 5022
- 5023
- 5024
- 5025
- 5026
- 5027
- 5028
- 5029
- 5030
- 5031
- 5032
- 5033
- 5034
- 5035
- 5036
- 5037
- 5038
- 5039
- 5040
- 5041
- 5042
- 5043
- 5044
- 5045
- 5046
- 5047
- 5048
- 5049
- 5050
- 5051
- 5052
- 5053
- 5054
- 5055
- 5056
- 5057
- 5058
- 5059
- 5060
- 5061
- 5062
- 5063
- 5064
- 5065
- 5066
- 5067
- 5068
- 5069
- 5070
- 5071
- 5072
- 5073
- 5074
- 5075
- 5076
- 5077
- 5078
- 5079
- 5080
- 5081
- 5082
- 5083
- 5084
- 5085
- 5086
- 5087
- 5088
- 5089
- 5090
- 5091
- 5092
- 5093
- 5094
- 5095
- 5096
- 5097
- 5098
- 5099
- 5100
- 5101
- 5102
- 5103
- 5104
- 5105
- 5106
- 5107
- 5108
- 5109
- 5110
- 5111
- 5112
- 5113
- 5114
- 5115
- 5116
- 5117
- 5118
- 5119
- 5120
- 5121
- 5122
- 5123
- 5124
- 5125
- 5126
- 5127
- 5128
- 5129
- 5130
- 5131
- 5132
- 5133
- 5134
- 5135
- 5136
- 5137
- 5138
- 5139
- 5140
- 5141
- 5142
- 5143
- 5144
- 5145
- 5146
- 5147
- 5148
- 5149
- 5150
- 5151
- 5152
- 5153
- 5154
- 5155
- 5156
- 5157
- 5158
- 5159
- 5160
- 5161
- 5162
- 5163
- 5164
- 5165
- 5166
- 5167
- 5168
- 5169
- 5170
- 5171
- 5172
- 5173
- 5174
- 5175
- 5176
- 5177
- 5178
- 5179
- 5180
- 5181
- 5182
- 5183
- 5184
- 5185
- 5186
- 5187
- 5188
- 5189
- 5190
- 5191
- 5192
- 5193
- 5194
- 5195
- 5196
- 5197
- 5198
- 5199
- 5200
- 5201
- 5202
- 5203
- 5204
- 5205
- 5206
- 5207
- 5208
- 5209
- 5210
- 5211
- 5212
- 5213
- 5214
- 5215
- 5216
- 5217
- 5218
- 5219
- 5220
- 5221
- 5222
- 5223
- 5224
- 5225
- 5226
- 5227
- 5228
- 5229
- 5230
- 5231
- 5232
- 5233
- 5234
- 5235
- 5236
- 5237
- 5238
- 5239
- 5240
- 5241
- 5242
- 5243
- 5244
- 5245
- 5246
- 5247
- 5248
- 5249
- 5250
- 5251
- 5252
- 5253
- 5254
- 5255
- 5256
- 5257
- 5258
- 5259
- 5260
- 5261
- 5262
- 5263
- 5264
- 5265
- 5266
- 5267
- 5268
- 5269
- 5270
- 5271
- 5272
- 5273
- 5274
- 5275
- 5276
- 5277
- 5278
- 5279
- 5280
- 5281
- 5282
- 5283
- 5284
- 5285
- 5286
- 5287
- 5288
- 5289
- 5290
- 5291
- 5292
- 5293
- 5294
- 5295
- 5296
- 5297
- 5298
- 5299
- 5300
- 5301
- 5302
- 5303
- 5304
- 5305
- 5306
- 5307
- 5308
- 5309
- 5310
- 5311
- 5312
- 5313
- 5314
- 5315
- 5316
- 5317
- 5318
- 5319
- 5320
- 5321
- 5322
- 5323
- 5324
- 5325
- 5326
- 5327
- 5328
- 5329
- 5330
- 5331
- 5332
- 5333
- 5334
- 5335
- 5336
- 5337
- 5338
- 5339
- 5340
- 5341
- 5342
- 5343
- 5344
- 5345
- 5346
- 5347
- 5348
- 5349
- 5350
- 5351
- 5352
- 5353
- 5354
- 5355
- 5356
- 5357
- 5358
- 5359
- 5360
- 5361
- 5362
- 5363
- 5364
- 5365
- 5366
- 5367
- 5368
- 5369
- 5370
- 5371
- 5372
- 5373
- 5374
- 5375
- 5376
- 5377
- 5378
- 5379
- 5380
- 5381
- 5382
- 5383
- 5384
- 5385
- 5386
- 5387
- 5388
- 5389
- 5390
- 5391
- 5392
- 5393
- 5394
- 5395
- 5396
- 5397
- 5398
- 5399
- 5400
- 5401
- 5402
- 5403
- 5404
- 5405
- 5406
- 5407
- 5408
- 5409
- 5410
- 5411
- 5412
- 5413
- 5414
- 5415
- 5416
- 5417
- 5418
- 5419
- 5420
- 5421
- 5422
- 5423
- 5424
- 5425
- 5426
- 5427
- 5428
- 5429
- 5430
- 5431
- 5432
- 5433
- 5434
- 5435
- 5436
- 5437
- 5438
- 5439
- 5440
- 5441
- 5442
- 5443
- 5444
- 5445
- 5446
- 5447
- 5448
- 5449
- 5450
- 5451
- 5452
- 5453
- 5454
- 5455
- 5456
- 5457
- 5458
- 5459
- 5460
- 5461
- 5462
- 5463
- 5464
- 5465
- 5466
- 5467
- 5468
- 5469
- 5470
- 5471
- 5472
- 5473
- 5474
- 5475
- 5476
- 5477
- 5478
- 5479
- 5480
- 5481
- 5482
- 5483
- 5484
- 5485
- 5486
- 5487
- 5488
- 5489
- 5490
- 5491
- 5492
- 5493
- 5494
- 5495
- 5496
- 5497
- 5498
- 5499
