NGC 1003
NGC 1003 is an Sc spiral galaxy located in the Perseus constellation about 28 million light years from the Milky Way.[4] It was discovered by the German-British astronomer William Herschel in 1784.[5] It is a member of the NGC 1023 Group.[3] A supernova was discovered in the galaxy in 1937, labeled SN 1937d.[6]
| NGC 1003 | |
|---|---|
 NGC 1003 as seen through the Hubble Space telescope. | |
| Observation data (J2000[1] epoch) | |
| Constellation | Perseus |
| Right ascension | 02h 39m 16.4s[1] |
| Declination | +40° 52′ 22″[1] |
| Redshift | 0.002090[2] |
| Helio radial velocity | 626 km/s[2] |
| Group or cluster | NGC 1023 Group[3] |
| Apparent magnitude (B) | 12.1[2] |
| Characteristics | |
| Type | SA(s)cd[2] |
See also
References
- "NGC 1003, Spiral Galaxy". Retrieved 1 April 2016.
- "NGC 1003". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-16.
- Trentham, Neil; Tully, R. Brent (2009). "Dwarf galaxies in the NGC 1023 Group". Monthly Notices of the Royal Astronomical Society. 398 (2): 722. arXiv:0906.2540. Bibcode:2009MNRAS.398..722T. doi:10.1111/j.1365-2966.2009.15189.x.
- "Revised NGC Data for NGC 1003". spider.seds.org. Retrieved 2017-09-17.
- "Your NED Search Results". nedwww.ipac.caltech.edu. Retrieved 2017-09-17.
- "1938ApJ....88..411B Page 411". adsabs.harvard.edu. Retrieved 2020-06-17.
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