NGC 1279 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Perseus |
Right ascension | 3h 19m 59.1s[1] |
Declination | 41° 28′ 46″[1] |
Redshift | 0.024300[1] |
Heliocentric radial velocity | 7285 km/s |
Distance | 317 Mly (97.1 Mpc)[1] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 15.5[1] |
Characteristics | |
Type | S/S0?[1] |
Size | ~113,400 ly (34.77 kpc) (estimated)[1] |
Apparent size (V) | 0.587 x 0.329[2] |
Other designations | |
PGC 12448, PGC 12449, 2MASX J03195907+4128462[1] |
NGC 1279 is a lenticular galaxy estimated to be 324 million light-years away from the Milky Way[3] in the constellation Perseus.[4] It has diameter of about 110,000 ly,[3] and is a member of the Perseus Cluster.[5][6]
It was discovered on December 12, 1876, by astronomer John Louis Emil Dreyer.[6]
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Transcription
References
- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 1279. Retrieved 2018-07-02.
- ^ "NGC 1279". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-02.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-07-02.
- ^ "Revised NGC Data for NGC 1279". spider.seds.org. Retrieved 2018-07-02.
- ^ Brunzendorf, J.; Meusinger, H. (October 1, 1999). "The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types". Astronomy and Astrophysics Supplement Series. 139 (1): 141–161. Bibcode:1999A&AS..139..141B. doi:10.1051/aas:1999111. ISSN 0365-0138.
- ^ a b "New General Catalog Objects: NGC 1250 - 1299".