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NGC 7513

NGC 7513
NGC 7513 by Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationSculptor
Right ascension23h 13m 14.0s[1]
Declination−28° 21′ 27″[1]
Redshift0.005217 ± 0.000013 [1]
Heliocentric radial velocity1,564 ± 4 km/s[1]
Distance62.4 ± 6.4 Mly (19.1 ± 2.0 Mpc)[1]
Apparent magnitude (V)11.3
Characteristics
Type(R')SB(s)b pec [1]
Apparent size (V)3.2′ × 2.1′[1]
Other designations
ESO 469- G022, AM 2310-283B, MCG -05-54-023, PGC 70714[1]

NGC 7513 is a barred spiral galaxy located in the constellation Sculptor. It is located at a distance of circa 62.5 million light years from Earth, which, given its apparent dimensions, means that NGC 7513 is about 75,000 light years across.[1] It was discovered by Albert Marth on September 24, 1864.[2]

A large star cluster has been found in the nucleus, with an estimated mass of 107.0 M☉.[3] There is circumnuclear dust distributed irregularly.[4]

NGC 7513 is a member of the NGC 7507 galaxy group, named after NGC 7507, along with some smaller galaxies.[5] NGC 7507 is an elliptical galaxy lying at a projected distance of 18 arcminutes.[6]

References

  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 7513. Retrieved 2019-01-18.
  2. ^ Seligman, Courtney. "NGC 7513 (= PGC 70714)". Celestial Atlas. Retrieved 19 November 2018.
  3. ^ Seth, Anil; Agüeros, Marcel; Lee, Duane; Basu-Zych, Antara (May 2008). "The Coincidence of Nuclear Star Clusters and Active Galactic Nuclei". The Astrophysical Journal. 678 (1): 116–130. arXiv:0801.0439. Bibcode:2008ApJ...678..116S. doi:10.1086/528955.
  4. ^ Carollo, C. Marcella; Stiavelli, Massimo; Seigar, Marc; de Zeeuw, P. Tim; Dejonghe, Herwig (January 2002). "Spiral Galaxies with HST/NICMOS. I. Nuclear Morphologies, Color Maps, and Distinct Nuclei". The Astronomical Journal. 123 (1): 159–183. arXiv:astro-ph/0110281. Bibcode:2002AJ....123..159C. doi:10.1086/324725.
  5. ^ 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.
  6. ^ Caso, J. P.; Richtler, T.; Bassino, L. P.; Salinas, R.; Lane, R. R.; Romanowsky, A. (July 2013). "The paucity of globular clusters around the field elliptical NGC 7507". Astronomy & Astrophysics. 555: A56. arXiv:1305.1335. Bibcode:2013A&A...555A..56C. doi:10.1051/0004-6361/201321032.
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