| NGC 3319 | |
|---|---|
.jpg)
SDSS image of NGC 3319 | |
| Observation data ( J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 10h 39m 09.533s [1] |
| Declination | +41° 41′ 12.74″ [1] |
| Redshift | 0.002420 [2] |
| Heliocentric radial velocity | 725 ± 5 km/s [2] |
| Distance | 46.6 ± 3.6 Mly (14.3 ± 1.1 Mpc) [3] |
| Apparent magnitude (V) | 11.07 [4] |
| Apparent magnitude (B) | 11.48 [4] |
| Characteristics | |
| Type | SB(rs)cd [4] |
| Apparent size (V) | 6.2′ × 3.4′ [4] |
| Other designations | |
| UGC 5789, MCG +07-22-036, PGC 31671 [2] | |
NGC 3319 is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on Feb 3, 1788. [5] It is rich in gas and lacks a galactic bulge. [3]
NGC 3319 is relatively isolated. It is in a small group of galaxies including NGC 3104, NGC 3184, and NGC 3198. The nearest galaxy to it is probably NGC 3198, 4.2 million light-years (1.3 megaparsecs) away. [3]
NGC 3319 is a Seyfert galaxy, with an active galactic nucleus (AGN) that was identified in 2018. [6] NGC 3319 is a candidate for hosting an intermediate-mass black hole. The probability of having the black hole having a mass less than 105 M☉ has been placed at 84%. [3]
Gallery
-
Pan-STARRS image of NGC 3319
References
- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode: 2006AJ....131.1163S. doi: 10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c "NGC 3319". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-21.
- ^ a b c d Davis, Benjamin L.; Graham, Alister W. (2021). "Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319". Publications of the Astronomical Society of Australia. 38. arXiv: 2105.04717. Bibcode: 2021PASA...38...30D. doi: 10.1017/pasa.2021.23. S2CID 234357763.
- ^ a b c d Gil de Paz, Armando; et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies". The Astrophysical Journal Supplement Series. 173 (2): 185–255. arXiv: astro-ph/0606440. Bibcode: 2007ApJS..173..185G. doi: 10.1086/516636. S2CID 119085482.
- ^ Seligman, Courtney. "New General Catalog Objects: NGC 3300 - 3349". cseligman.com. Retrieved 3 April 2019.
- ^ Jiang, Ning; Wang, Tinggui; Zhou, Hongyan; Shu, Xinwen; Yang, Chenwei; Dou, Liming; Sun, Luming; Dong, Xiaobo; Wang, Shaoshao; Yang, Huan (2018). "Discovery of an Active Intermediate-mass Black Hole Candidate in the Barred Bulgeless Galaxy NGC 3319". The Astrophysical Journal. 869 (1): 49. arXiv: 1810.10283. Bibcode: 2018ApJ...869...49J. doi: 10.3847/1538-4357/aaeb90. S2CID 119048841.
External links
-
Media related to
NGC 3319 at Wikimedia Commons
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |
| NGC 3319 | |
|---|---|
|
SDSS image of NGC 3319 | |
| Observation data ( J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 10h 39m 09.533s [1] |
| Declination | +41° 41′ 12.74″ [1] |
| Redshift | 0.002420 [2] |
| Heliocentric radial velocity | 725 ± 5 km/s [2] |
| Distance | 46.6 ± 3.6 Mly (14.3 ± 1.1 Mpc) [3] |
| Apparent magnitude (V) | 11.07 [4] |
| Apparent magnitude (B) | 11.48 [4] |
| Characteristics | |
| Type | SB(rs)cd [4] |
| Apparent size (V) | 6.2′ × 3.4′ [4] |
| Other designations | |
| UGC 5789, MCG +07-22-036, PGC 31671 [2] | |
NGC 3319 is a barred spiral galaxy in the constellation Ursa Major. It was discovered by William Herschel on Feb 3, 1788. [5] It is rich in gas and lacks a galactic bulge. [3]
NGC 3319 is relatively isolated. It is in a small group of galaxies including NGC 3104, NGC 3184, and NGC 3198. The nearest galaxy to it is probably NGC 3198, 4.2 million light-years (1.3 megaparsecs) away. [3]
NGC 3319 is a Seyfert galaxy, with an active galactic nucleus (AGN) that was identified in 2018. [6] NGC 3319 is a candidate for hosting an intermediate-mass black hole. The probability of having the black hole having a mass less than 105 M☉ has been placed at 84%. [3]
Gallery
-
Pan-STARRS image of NGC 3319
References
- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode: 2006AJ....131.1163S. doi: 10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c "NGC 3319". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-21.
- ^ a b c d Davis, Benjamin L.; Graham, Alister W. (2021). "Refining the mass estimate for the intermediate-mass black hole candidate in NGC 3319". Publications of the Astronomical Society of Australia. 38. arXiv: 2105.04717. Bibcode: 2021PASA...38...30D. doi: 10.1017/pasa.2021.23. S2CID 234357763.
- ^ a b c d Gil de Paz, Armando; et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies". The Astrophysical Journal Supplement Series. 173 (2): 185–255. arXiv: astro-ph/0606440. Bibcode: 2007ApJS..173..185G. doi: 10.1086/516636. S2CID 119085482.
- ^ Seligman, Courtney. "New General Catalog Objects: NGC 3300 - 3349". cseligman.com. Retrieved 3 April 2019.
- ^ Jiang, Ning; Wang, Tinggui; Zhou, Hongyan; Shu, Xinwen; Yang, Chenwei; Dou, Liming; Sun, Luming; Dong, Xiaobo; Wang, Shaoshao; Yang, Huan (2018). "Discovery of an Active Intermediate-mass Black Hole Candidate in the Barred Bulgeless Galaxy NGC 3319". The Astrophysical Journal. 869 (1): 49. arXiv: 1810.10283. Bibcode: 2018ApJ...869...49J. doi: 10.3847/1538-4357/aaeb90. S2CID 119048841.
External links
-
Media related to
NGC 3319 at Wikimedia Commons
|
| This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |