NGC 7513

NGC 7513
NGC 7513 by Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationSculptor
Right ascension23h 13m 14.0s
Declination−28° 21′ 27″
Redshift0.005217 ± 0.000013
Heliocentric radial velocity1,564 ± 4 km/s
Distance62.4 ± 6.4 Mly (19.1 ± 2.0 Mpc)
Apparent magnitude (V)11.3
Characteristics
Type(R')SB(s)b pec
Apparent size (V)3.2′ × 2.1′
Other designations
UGCA 437, ESO 469- G022, AM 2310-283B, MCG -05-54-023, PGC 70714

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. It was discovered by Albert Marth on September 24, 1864.

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

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

References

  1. 1 2 3 4 5 6 7 8 9 "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.