Astronomy:NGC 1015

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NGC 1015
NGC 1015 imaged by the Hubble Space Telescope[1]
Observation data (J2000[2] epoch)
ConstellationCetus
Right ascension 02h 38m 11.552s[3]
Declination−01° 19′ 07.60″[3]
Redshift0.008776(4)[4]
Helio radial velocity2625.7km/s[5]
Distance118 Mly (36.3 Mpc)[6]
Apparent magnitude (B)12.8[2]
Characteristics
TypeSb[7]
Apparent size (V)163.88″[7]
Other designations
UGC 2124, MCG+00-07-066[2]

NGC 1015 is a barred spiral galaxy,[7] at a distance of 118 million light years[6] in the constellation of Cetus (The Whale).[1] It was discovered by German astronomer Wilhelm Tempel on 27 December 1875.[8] Emissions from the core region satisfy the criteria for an active galactic nucleus of type 2 Seyfert and a LINER galaxy.[9]

Supernova

One supernova has been observed in NGC 1015. SN 2009ig (Type Ia,[7] mag. 17.5) was discovered by the Lick Observatory Supernova Search (LOSS) on 20 August 2009.[10][11][12] It got as bright as magnitude 13, making it the brightest supernova of 2009.[13]

See also

  • List of NGC objects (1001-2000)

References

  1. ↑ 1.0 1.1 "Spirals and supernovae". https://www.spacetelescope.org/images/potw1811a/. 
  2. ↑ 2.0 2.1 2.2 "NGC 1015". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+1015. 
  3. ↑ 3.0 3.1 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  4. ↑ de Vaucouleurs, G. (1991). Third reference catalogue of bright galaxies. New York: Springer-Verlag. 
  5. ↑ Meyer, M. J. (June 2004). "The HIPASS catalogue - I. Data presentation". Monthly Notices of the Royal Astronomical Society 350 (4): 1195–1209. doi:10.1111/j.1365-2966.2004.07710.x. Bibcode: 2004MNRAS.350.1195M. 
  6. ↑ 6.0 6.1 Cappellari, Michele (May 11, 2011). "The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria". Monthly Notices of the Royal Astronomical Society 413 (2): 813–836. doi:10.1111/j.1365-2966.2010.18174.x. Bibcode: 2011MNRAS.413..813C. 
  7. ↑ 7.0 7.1 7.2 7.3 Hakobyan, A. A. (March 2016). "Supernovae and their host galaxies - III. The impact of bars and bulges on the radial distribution of supernovae in disc galaxies". Monthly Notices of the Royal Astronomical Society 456 (3): 2848–2860. doi:10.1093/mnras/stv2853. Bibcode: 2016MNRAS.456.2848H. 
  8. ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 1015". https://cseligman.com/text/atlas/ngc10.htm#1015. 
  9. ↑ Chen, Yan-Ping et al. (January 2022). "A Uniformly Selected, Southern-sky 6dF, Optical AGN Catalog" (in en). The Astrophysical Journal Supplement Series 258 (2): 29. doi:10.3847/1538-4365/ac4157. ISSN 0067-0049. Bibcode: 2022ApJS..258...29C. 
  10. ↑ Kleiser, I. et al. (2009). "Supernova 2009ig in NGC 1015". Central Bureau Electronic Telegrams (1918): 1. Bibcode: 2009CBET.1918....1K. http://www.cbat.eps.harvard.edu/cbet/001900/CBET001918.txt. 
  11. ↑ Foley, Ryan J. et al. (January 2012). "Very Early Ultraviolet and Optical Observations of the Type Ia Supernova 2009ig". The Astrophysical Journal 744 (1): 38. doi:10.1088/0004-637X/744/1/38. ISSN 0004-637X. Bibcode: 2012ApJ...744...38F. 
  12. ↑ "SN 2009ig". IAU. https://www.wis-tns.org/object/2009ig. 
  13. ↑ Bishop, David. "Bright Supernovae - 2009". https://www.rochesterastronomy.org/sn2009/index.html. 

Template:NGC objects:1001-2000

Coordinates: Sky map 02h 38m 11.565s, -01° 19′ 07.02″



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