NGC 1819 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Orion |
Right ascension | 05h 11m 46.150s[1] |
Declination | +05° 12′ 02.21″[1] |
Redshift | 0.014880±0.000047[2] |
Heliocentric radial velocity | 4,483[2] km/s |
Distance | 197.4 Mly (60.53 Mpc)[3] |
Apparent magnitude (V) | 13[4] |
Surface brightness | 23.34 mag/arcsec2[citation needed] |
Characteristics | |
Type | SB0[5] |
Other designations | |
IRAS 05091+0508, UGC 3265, MCG -1-14-2, PGC 16899[6] |
NGC 1819 is a lenticular galaxy in the constellation of Orion.[4] It was discovered on December 26, 1885, by American astronomer Lewis A. Swift.[7] This galaxy is located at a distance of 197.4 million light-years (60.53 Mpc) from the Milky Way,[3] and is receding with a heliocentric radial velocity of 4,483 km/s.[2]
The morphological classification of NGC 1819 is SB0 in the De Vaucouleurs system,[5] indicating this is a lenticular galaxy with a barred spiral organization. It is a gas-rich galaxy[8] with a circumnuclear ring structure that is undergoing intense star formation.[9]
Type Ia supernova[5] SN 2005el was discovered in NGC 1819 on September 19, 2005. It was positioned 39.0″ east and 22.6″ south of the nucleus.[10]
Skrutskie_et_al_2006
was invoked but never defined (see the help page).Paturel2002
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was invoked but never defined (see the help page).SEDS
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was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).CSeligman
was invoked but never defined (see the help page).Pogge_Eskridge_1993
was invoked but never defined (see the help page).Contini_et_al_1995
was invoked but never defined (see the help page).Madison_et_al_2005
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