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NGC 2985

From Wikipedia, the free encyclopedia
Galaxy in the constellation Ursa Major
NGC 2985
Observation data (J2000epoch)
ConstellationUrsa Major
Right ascension09h 50m 22.2s[2]
Declination+72° 16′ 43″[2]
Redshift0.004410 ± 0.0000237[2]
Heliocentric radial velocity1,322 ± 7km/s[2]
Distance70.1 ± 4.1Mly (21.5 ± 1.3Mpc)[2]
Apparent magnitude (V)10.4[3]
Characteristics
Type(R')SA(rs)ab[2]
Apparent size (V)4.6 × 3.6[2]
Other designations
UGC 5253, CGCG 332-067,MCG +12-10-006,PGC 28316[2]

NGC 2985 is aspiral galaxy located in the constellationUrsa Major. It is located at a distance of circa 70 millionlight years from Earth, which, given its apparent dimensions, means that NGC 2985 is about 95,000 light years across. It was discovered byWilliam Herschel on April 3, 1785.[4]

The galaxy is seen with an inclination of 37 degrees.[5] The galaxy has a bright nucleus from which emanate multiple tightly woundspiral fragments.[6] Numerous blue knots are visible at thegalactic disk. At the outer part of the galaxy lies a massive spiral arm that forms a pseudoring that encircles the galaxy. The inner part of the galaxy, where activestar formation has been observed, has been found to be unstable, contrary to the outer stable one. It has been suggested that the presence ofmolecular clouds accounts for the instability of the region.[5]

The nucleus of NGC 2985 isactive, and based on its spectrum has been categorised as aLINER. The most accepted theory for the activity source is the presence of anaccretion disk around a supermassive black hole. The mass of the supermassive black hole at the centre of NGC 2985 is estimated to be 160 million (108.2)M, based on stellarvelocity dispersion.[7] The velocity dispersion isanisotropic, and changes with theazimuth. The rotational speed of the galaxy at itseffective radius is 222.9 ± 31.2 km/s.[8]

NGC 2985 is the brightest member of agalaxy group known as the NGC 2985 group. Other members of the group includeNGC 3027, 25 arcminutes away. Other nearby galaxies includeNGC 3252, andNGC 3403.[9]

References

[edit]
  1. ^"A Beautiful Whorl".www.spacetelescope.org. Retrieved15 July 2019.
  2. ^abcdefgh"NASA/IPAC Extragalactic Database".Results for NGC 2985. Retrieved2019-01-18.
  3. ^"Revised NGC Data for NGC 2985".spider.seds.org. Retrieved25 November 2018.
  4. ^Seligman, Courtney."NGC 2985 (= PGC 28316)".Celestial Atlas. Retrieved19 November 2018.
  5. ^abMarchuk, A A; Sotnikova, N Y (April 2018)."Two-component gravitational instability in spiral galaxies".Monthly Notices of the Royal Astronomical Society.475 (4):4891–4910.arXiv:1804.07962.Bibcode:2018MNRAS.475.4891M.doi:10.1093/mnras/sty100.S2CID 86864987.
  6. ^Sandage, A., Bedke, J. (1994),The Carnegie Atlas of Galaxies. Volume I, Carnegie Institution of Washington
  7. ^Dong, X. Y.; De Robertis, M. M. (March 2006). "Low-Luminosity Active Galaxies and Their Central Black Holes".The Astronomical Journal.131 (3):1236–1252.arXiv:astro-ph/0510694.Bibcode:2006AJ....131.1236D.doi:10.1086/499334.S2CID 17630682.
  8. ^Noordermeer, E.; Merrifield, M. R.; Aragn-Salamanca, A. (June 2008)."Exploring disc galaxy dynamics using integral field unit data".Monthly Notices of the Royal Astronomical Society.388 (3):1381–1393.arXiv:0805.3230.Bibcode:2008MNRAS.388.1381N.doi:10.1111/j.1365-2966.2008.13487.x.S2CID 18059212.
  9. ^Makarov, Dmitry; Karachentsev, Igor (21 April 2011)."Galaxy groups and clouds in the local (z~ 0.01) Universe".Monthly Notices of the Royal Astronomical Society.412 (4):2498–2520.arXiv:1011.6277.Bibcode:2011MNRAS.412.2498M.doi:10.1111/j.1365-2966.2010.18071.x.S2CID 119194025.

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