NGC 1559 | |
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![]() NGC 1559 imaged by the Hubble Space Telescope | |
Observation data (J2000.0 epoch) | |
Constellation | Reticulum |
Right ascension | 04h 17m 35.7506s [1] |
Declination | −62° 47′ 01.316″ [1] |
Redshift | 1304 ± 4 km/s [1] |
Distance | 48.73 ± 2.18 Mly (14.942 ± 0.669 Mpc) [1] |
Apparent magnitude (V) | 11 [1] |
Characteristics | |
Type | SB(s)cd [1] |
Size | ~75,600 ly (23.17 kpc) (estimated) [1] |
Apparent size (V) | 3.5′ × 2.0′ [1] |
Other designations | |
ESO 084- G 010, IRAS 04170-6253, 2MASX J04173578-6247012, PGC 14814 [1] |
NGC 1559 is a barred spiral galaxy in the constellation Reticulum. It was discovered on 6 November 1826 by Scottish astronomer James Dunlop. [2]
NGC 1559 is a Seyfert galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. Although it was originally thought to be a member of the Dorado Group, [3] subsequent observations have shown that it is in fact not a member of any galaxy group or cluster and does not have any nearby companions. [4] [5] NGC 1559 has massive spiral arms and strong star formation. [4] It contains a small bar which is oriented nearly east-west and spans 40″. [4] Its bar and disc are the source of very strong radio emissions. [4]
Four supernovae have been observed in NGC 1559: