NGC 4451 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 28m 40.558s[1] |
Declination | 09° 15′ 32.13″[1] |
Redshift | 0.002882[2] |
Heliocentric radial velocity | 862[3] |
Distance | 85.0 Mly (26.06 Mpc)[4] |
Group or cluster | Virgo cluster |
Apparent magnitude (V) | 13.29[2] |
Characteristics | |
Type | SA(rs)cd[5] |
Mass | 8.2+8.2 −3.1[4] M☉ |
Apparent size (V) | 1.5′ × 1.0′[2] |
Half-light radius (apparent) | 11.86″[6] |
Other designations | |
NGC 4451, UGC 7600, MCG +02-32-079, PGC 41050[7] |
NGC 4451 is a spiral galaxy in the equatorial Virgo constellation. It was discovered at the Copenhagen Observatory on March 19, 1865, by Heinrich d'Arrest, who used an 11" refractor telescope.[8] The galaxy is located at a distance of 85[4] million light years and is receding with a heliocentric radial velocity of 862 km/s.[3] It is a member of the Virgo cluster of galaxies.[6]
In March 1985, Shigo Horiguchi in Japan[9] discovered a Type II-P supernova[10] in this galaxy. Designated SN 1985G, it was positioned 2″ west and 5″ north of the galaxy center.[9] The progenitor was estimated to have a mass of 21.7+4.4
−0.5 M☉ and was 8.65+0.14
−1.34[10] million years old.
Skrutskie_et_al_2006
was invoked but never defined (see the help page).ned
was invoked but never defined (see the help page).Tully_et_al_2016
was invoked but never defined (see the help page).Lianou_et_al_2019
was invoked but never defined (see the help page).Buta2019
was invoked but never defined (see the help page).Kim_et_al_2014
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).discovery
was invoked but never defined (see the help page).Kozai_Horiguchi_1985
was invoked but never defined (see the help page).Kuncarayakti_et_al_2018
was invoked but never defined (see the help page).