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) | |
Constellation | Leo Minor |
Right ascension | 11h 03m 11.2s[1] |
Declination | +27° 58′ 21″[1] |
Redshift | 1534 ± 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]
{{cite book}}
: CS1 maint: multiple names: authors list (link)