NGC 1015
NGC 1015, as taken by Hubble Space Telescope[1]
Observation data (J2000[2] epoch)
ConstellationCetus
Right ascension02h 38m 11.565s[2]
Declination−01° 19 07.02[2]
Redshift0.008797[2]
Heliocentric radial velocity2625.7km/s[2]
Apparent magnitude (B)12.8[2]
Characteristics
TypeSb[2]
Other designations
6dFGS gJ023811.6-011907, HIPASS J0238-01, LEDA 9988, 2MASX J02381156-0119070, MCG+00-07-066, SDSS J023811.55-011907.5, UGC 2124, UZC J023811.5-011908, Z 388-75, Z 0235.6-0132, [PVK2003] 039.54833 -01.31778[2]

NGC 1015 is a barred spiral galaxy that is located at distance of 118 million light years away from earth in the constellation of Cetus (The Whale). The galaxy's most notable feature is its fairly large and bright center with smooth, tightly wounded spiral arms.[1] The distance modulus to NGC 1015 is equal to the distance to NGC 1015 in Mpc. The galaxy was discovered on December 27 in the year 1875 by the German astronomer Wilhelm Temple.[3]

The galaxy is host to SN 2009ig, a typical Type Ia supernova.[4]

See also

References

  1. 1 2 "Spirals and supernovae". www.spacetelescope.org. Retrieved 13 March 2018.
  2. 1 2 3 4 5 6 7 8 "SIMBAD Astronomical Database – CDS (Strasbourg)". Results for NGC 1015. Retrieved 2018-03-13.
  3. Staff, News (2018-03-12). "Hubble Space Telescope Looks at Stunning Spiral Galaxy: NGC 1015 | Astronomy | Sci-News.com". Sci.News: Breaking Science News. Retrieved 2023-11-26. {{cite web}}: |first= has generic name (help)
  4. Foley, Ryan J.; Challis, P. J.; Filippenko, A. V.; Ganeshalingam, M.; Landsman, W.; Li, W.; Marion, G. H.; Silverman, J. M.; Beaton, R. L.; Bennert, V. N.; Cenko, S. B. (2012-01-01). "Very Early Ultraviolet and Optical Observations of the Type Ia Supernova 2009ig". The Astrophysical Journal. 744 (1): 38. arXiv:1109.0987. Bibcode:2012ApJ...744...38F. doi:10.1088/0004-637X/744/1/38. hdl:2152/34649. ISSN 0004-637X. S2CID 119200461.


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