NGC 1019 | |
---|---|
Observation data (J2000.0 epoch) | |
Constellation | Cetus |
Right ascension | 02h 38m 27.41s[1] |
Declination | +01° 54′ 27.79″[1] |
Redshift | 0.024340[1] |
Heliocentric radial velocity | 7297 ± 20 km/s[1] |
Distance | 316 Mly[2] |
Apparent magnitude (V) | 13.60[3] |
Apparent magnitude (B) | 14.40[3] |
Characteristics | |
Type | SB(rs)bc[1] |
Apparent size (V) | 1.0 × 0.9[1] |
Other designations | |
UGC 2132, MCG +0-7-68, PGC 10006 |
NGC 1019 is a barred spiral galaxy approximately 316 million light-years away from Earth in the constellation of Cetus.[2] It was discovered by French astronomer Édouard Stephan on December 1, 1880 with the 31" reflecting telescope at the Marseille Observatory.[4]
NGC 1019 is classified as Type I Seyfert galaxy.[2] Its nuclei is surrounded by tight rings or annuli of star formation,[5] and the rings contain compact, young star clusters.[6]
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