NGC 1819
Appearance
NGC 1819 | |
---|---|
![]() Pan-STARRSimage of NGC 1819 | |
Observation data | |
Constellation | Orion |
Right ascension | 05h11m46.150s[1] |
Declination | +05° 12′ 02.21″[1] |
Redshift | 0.014880±0.000047[2] |
Heliocentric radial velocity | 4,483[2]km/s |
Distance | 197.4Mly(60.53Mpc)[3] |
Apparent magnitude(V) | 13[4] |
Surface brightness | 23.34 mag/arcsec2[citation needed] |
Characteristics | |
Type | SB0[5] |
Other designations | |
IRAS05091+0508,UGC3265,MCG-1-14-2,PGC16899[6] |
NGC 1819is alenticular galaxyin theconstellationofOrion.[4]It was discovered on December 26, 1885, by American astronomerLewis A. Swift.[7]This galaxy is located at a distance of 197.4 millionlight-years(60.53Mpc) from theMilky Way,[3]and is receding with a heliocentricradial velocityof4,483 km/s.[2]
Themorphological classificationof 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 intensestar formation.[9]
Type Ia supernova[5]SN 2005elwas discovered in NGC 1819 on September 19, 2005. It was positioned39.0″east and22.6″south of the nucleus.[10]
References
[edit]- ^abSkrutskie, Michael F.; et al. (February 1, 2006)."The Two Micron All Sky Survey (2MASS)".The Astronomical Journal.131(2): 1163–1183.Bibcode:2006AJ....131.1163S.doi:10.1086/498708.ISSN0004-6256.S2CID18913331.
- ^abcPaturel, G.; et al. (2002). "Comparison LEDA/SIMBAD octobre 2002. Catalogue to be published in 2003".LEDA.Bibcode:2002LEDA.........0P.
- ^abTully, R. Brent; et al. (August 2016)."Cosmicflows-3".The Astronomical Journal.152(2): 21.arXiv:1605.01765.Bibcode:2016AJ....152...50T.doi:10.3847/0004-6256/152/2/50.S2CID250737862.50.
- ^abFrommert, Hartmut."NGC 1819".SEDS.Retrieved2024-04-05.
- ^abcKang, Yijung; et al. (March 2016)."Early-type Host Galaxies of Type Ia Supernovae. I. Evidence for Downsizing".The Astrophysical Journal Supplement Series.223(1). id. 7.arXiv:1601.05424.Bibcode:2016ApJS..223....7K.doi:10.3847/0067-0049/223/1/7.
- ^"NGC 1819".SIMBAD.Centre de données astronomiques de Strasbourg.Retrieved2019-05-22.
- ^Seligman, Courtney."NGC Objects: NGC 1800 - 1849".Celestial Atlas.Retrieved2024-04-05.
- ^Pogge, Richard W.; Eskridge, Paul B. (October 1993). "Star Formation in the Disks of H I-Rich SO Galaxies".Astronomical Journal.106:1405.Bibcode:1993AJ....106.1405P.doi:10.1086/116735.
- ^Contini, T.; et al. (1995). "Detection of circum-nuclear rings in barred spiral galaxies".Astrophysical Letters and Communications.31:223.Bibcode:1995ApL&C..31..223C.
- ^Madison, D. R.; et al. (September 2005). Green, D. W. E. (ed.). "Supernova 2005el in NGC 1819".Central Bureau Electronic Telegrams.233:1.Bibcode:2005CBET..233....1M.