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)
ConstellationPerseus
Right ascension02h 39m 16.4s[1]
Declination+40° 52′ 22″[1]
Redshift0.002090[2]
Helio radial velocity626 km/s[2]
Group or clusterNGC 1023 Group[3]
Apparent magnitude (B)12.1[2]
Characteristics
TypeSA(s)cd[2]

See also

References
  1. "NGC 1003, Spiral Galaxy". Retrieved 1 April 2016.
  2. "NGC 1003". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-16.
  3. 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.
  4. "Revised NGC Data for NGC 1003". spider.seds.org. Retrieved 2017-09-17.
  5. "Your NED Search Results". nedwww.ipac.caltech.edu. Retrieved 2017-09-17.
  6. "1938ApJ....88..411B Page 411". adsabs.harvard.edu. Retrieved 2020-06-17.
  7. "NGC 1003". noirlab.edu. Retrieved 5 January 2021.
  • Media related to NGC 1003 at Wikimedia Commons


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.