NGC 3504

Summary

NGC 3504 is a barred spiral galaxy in the constellation Leo Minor. It is a member of the NGC 3504 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[3]

NGC 3504
Observation data (J2000 epoch)
ConstellationLeo Minor
Right ascension11h 03m 11.2s[1]
Declination+27° 58′ 21″[1]
Redshift1534 ± 2 km/s[1]
Apparent magnitude (V)11.67[1]
Characteristics
Type(R)SAB(s)ab [1]
Apparent size (V)2.7 × 2.1[1]
Other designations
UGC 6118, MCG +05-26-039, PGC 33371[2]

There is a large amount of molecular gas centered on the galactic nucleus. Compared with other barred spiral galaxies, NGC 3504 is in an early phase of its evolution.[4]

The mass of NGC 3504 has been difficult to narrow down, but it is believed to be between 2.5*109 M⊙ and 9*109 M⊙.[5]

One supernovae has been observed in NGC 3504: SN 1998cf (type unknown, mag. 15).[6]

References edit

  1. ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for NGC 3504. Retrieved 2008-04-10.
  2. ^ "NGC 3504". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-23.
  3. ^ "The Leo III Groups". Atlas of the Universe. Archived from the original on July 22, 2012. Retrieved 2010-11-27.
  4. ^ Franco, J & F, Ferrini (1993). Star Formation, Galaxies and the Interstellar Medium. Cambridge University Press. ISBN 978-0-521-44412-5.{{cite book}}: CS1 maint: multiple names: authors list (link)
  5. ^ Burbidge; et al. (1960). "The Rotation and Approximate Mass of NGC 3504".
  6. ^ Transient Name Server entry for SN 1998cf. Retrieved 30 March 2023.

External links edit

  •   Media related to NGC 3504 at Wikimedia Commons
  • NGC 3504 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images