NGC 1276 is an optical[2][3] double star system[1][8][9][10] located in the constellation Perseus.[1][8][10] The system was discovered by astronomer John Dreyer[1][10][11] on December 12, 1876.[1][11] The pair consists of two 15th magnitude stars[1][4] known as Pul -3 270349 and Pul -3 270357 that are unrelated as they lie at different distances from each other.[4][2][3] Pul -3 270349 lies at a distance of 1,134.5587 parsecs (3,700.436 ly)[2] and Pul -3 270357 lies at a distance of 1,774.6229 parsecs (5,788.046 ly).[3]

The two stars are about the same size and luminosity as the Sun.[5]

See also

References

  1. ^ a b c d e f g h "New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 2021-06-05.
  2. ^ a b c d e f g h i j k "Pul -3 270349". simbad. Retrieved 2021-06-05.
  3. ^ a b c d e f g h i j k "Pul -3 270357". simbad. Retrieved 2021-06-05.
  4. ^ a b c d e f "coord 03 19 51.19730154413 41 38 29.0093822673 (ICRS, J2000, 2000.0), radius: .5 arcmin". simbad. Retrieved 2021-06-05.
  5. ^ a b c d e f g Brown, A. G. A.; Vallenari, A.; Prusti, T.; Bruijne, J. H. J. de; Babusiaux, C.; Bailer-Jones, C. a. L.; Biermann, M.; Evans, D. W.; Eyer, L.; Jansen, F.; Jordi, C. (2018-08-01). "Gaia Data Release 2 - Summary of the contents and survey properties". Astronomy & Astrophysics. 616: A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. hdl:2445/140475. ISSN 0004-6361.
  6. ^ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2021-06-05.
  7. ^ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2021-06-05.
  8. ^ a b "Revised NGC Data for NGC 1276". spider.seds.org. Retrieved 2021-06-05.
  9. ^ "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2021-06-05.
  10. ^ a b c "Notes on the NGC objects, particularly those missing, misidentified, or otherwise unusual (ngcnotes.all)". Historically-aware NGC/IC Positions and Notes. Retrieved 2021-06-04.
  11. ^ a b "Photos". www.klima-luft.de. Retrieved 2021-06-05.
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