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NGC 732

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Galaxy in constellation Andromeda
NGC 732
Pan-STARRS image of NGC 732
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension01 56 27.7
Declination36° 48′ 08″
Redshift0.019660
Heliocentric radial velocity5894 km/s
Distance250 Mly (77 Mpc)
Group or clusterAbell 262
Apparent magnitude (V)14.49
Characteristics
TypeS0
Size~120,000 ly (37 kpc) (estimated)
Apparent size (V)1.4 x 1.0
Other designations
Mrk 1011, MCG +06-05-057, PGC 007270, UGC 01406

NGC 732 is a lenticular galaxy located 250 million light-years away in the constellation Andromeda. It was discovered by astronomer Édouard Stephan on December 5, 1883 and is a member of Abell 262.

2017fpt

On July 20, 2017, a type Ia supernova designated as 2017fpt was discovered in NGC 732.

See also

References

  1. ^ "NASA/IPAC Extragalactic Database". Results for NGC 732. Retrieved 2018-12-29.
  2. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-29.
  3. "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
  4. "NGC 732". SIMBAD Astronomical Database. Retrieved 2018-12-30.
  5. Miller, Neal A.; Owen, Frazer N. (2001-06-01). "The Radio Galaxy Populations of Nearby Northern Abell Clusters". The Astrophysical Journal Supplement Series. 134 (2): 355–383. arXiv:astro-ph/0101114. Bibcode:2001ApJS..134..355M. doi:10.1086/320857. ISSN 0067-0049. S2CID 119052072.
  6. Petrosian, Artashes; McLean, Brian; Allen, Ronald J.; MacKenty, John W. (2007-05-01). "Markarian Galaxies. I. The Optical Database and Atlas". The Astrophysical Journal Supplement Series. 170 (1): 33–70. Bibcode:2007ApJS..170...33P. doi:10.1086/511333. ISSN 0067-0049. S2CID 8916810.
  7. "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-02-10.
  8. "Bright Supernovae - 2017". rochesterastronomy.org. Retrieved 2019-02-10.
  9. "2017fpt - The Open Supernova Catalog". Archived from the original on 2016-09-17. Retrieved 2019-02-10.
  10. "Gaia17bux". gsaweb.ast.cam.ac.uk. Retrieved 2019-02-10.

External links

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