Astronomy:NGC 1003

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Short description: Galaxy in the constellation Perseus
NGC 1003
NGC 1003 -HST09042 15-R814GB435.png
NGC 1003 from the Hubble Space Telescope
Observation data (J2000[1] epoch)
ConstellationPerseus
Right ascension 02h 39m 16.893s[2]
Declination+40° 52′ 20.25″[2]
Redshift0.002090[3]
Helio radial velocity624 km/s[4]
Distance35.9 kly (11.02 kpc)[4]
Group or clusterNGC 1023 group[5]
Apparent magnitude (B)12.1[3]
Characteristics
TypeSAcd[6]
Mass299+28
−26×1010[7] M☉
Mass/Light ratio0.70+0.16
−0.15[7] M☉/L☉
Notable featuresWarped disk[6]
Other designations
NGC 1003, UGC 2137, MCG+07-06-051, PGC 10052[3]

NGC 1003 is a spiral galaxy at the western edge of the Perseus constellation.[8] It is located at a distance of about 36 million light years from the Milky Way and is receding with a heliocentric radial velocity of 624 km/s.[4] This galaxy was discovered by the Anglo-German astronomer William Herschel on October 6, 1784, who described it as "pretty faint, large, extended 90°±, much brighter middle, mottled but not resolved".[9] It is a member of the NGC 1023 group of galaxies.[5]

The morphological class of NGC 1003 is SAcd, which means it is an unbarred spiral galaxy (SA) with somewhat loosely-wound spiral arms (cd). It is inclined by an angle of 70° to the line of sight from the Earth, with the major axis aligned along a position angle of 276°. The visual disk of the galaxy shows a substantial warping in the eastern side, turning it almost face on. The estimated star formation rate is 0.40 M☉·yr−1.[6] It has a virial mass of 3×1012 M☉ and a mass-to-light ratio of 0.7.[7]

A type Ia supernova[10] was discovered in the galaxy by F. Zwicky in 1937,[11] and subsequently designated SN 1937D.

Gallery

References

  1. ↑ "NGC 1003, Spiral Galaxy". http://www.kopernik.org/images/archive/n1003.htm. 
  2. ↑ 2.0 2.1 Skrutskie, Michael F. et al. (February 1, 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal 131 (2): 1163–1183. doi:10.1086/498708. ISSN 0004-6256. Bibcode: 2006AJ....131.1163S. 
  3. ↑ 3.0 3.1 3.2 "NGC 1003". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+1003. 
  4. ↑ 4.0 4.1 4.2 Tully, R. Brent et al. (August 2016). "Cosmicflows-3". The Astronomical Journal 152 (2): 21. doi:10.3847/0004-6256/152/2/50. 50. Bibcode: 2016AJ....152...50T. 
  5. ↑ 5.0 5.1 Trentham, Neil; Tully, R. Brent (2009). "Dwarf galaxies in the NGC 1023 Group". Monthly Notices of the Royal Astronomical Society 398 (2): 722. doi:10.1111/j.1365-2966.2009.15189.x. Bibcode: 2009MNRAS.398..722T. 
  6. ↑ 6.0 6.1 6.2 Marasco, A. et al. (November 2019). "HALOGAS: the properties of extraplanar HI in disc galaxies". Astronomy & Astrophysics 631: 27. doi:10.1051/0004-6361/201936338. A50. Bibcode: 2019A&A...631A..50M. 
  7. ↑ 7.0 7.1 7.2 Haghi, Hosein et al. (July 2018). "Rotation curves of galaxies and the stellar mass-to-light ratio". Monthly Notices of the Royal Astronomical Society 477 (3): 4187–4199. doi:10.1093/mnras/sty523. Bibcode: 2018MNRAS.477.4187H. 
  8. ↑ Sinnott, Roger W.; Perryman, Michael A. C. (1997). Millennium Star Atlas. 1. Sky Publishing Corporation and the European Space Agency. p. 100. ISBN 0-933346-84-0. 
  9. ↑ Seligman, Courtney. "NGC 1003 (= PGC 10052)". Celestial Atlas. https://cseligman.com/text/atlas/ngc10.htm#1003. 
  10. ↑ Navasardyan, H. et al. (December 2001). "Supernovae in isolated galaxies, in pairs and in groups of galaxies". Monthly Notices of the Royal Astronomical Society 328 (4): 1181–1192. doi:10.1046/j.1365-8711.2001.04942.x. Bibcode: 2001MNRAS.328.1181N. 
  11. ↑ Baade, W.; Zwicky, F. (November 1938). "Photographic Light-Curves of the Two Supernovae in IC 4182 and NGC 1003". Astrophysical Journal 88: 411. doi:10.1086/143996. Bibcode: 1938ApJ....88..411B. 
  12. ↑ "NGC 1003" (in en). https://noirlab.edu/public/images/noirlab2101a/. 

External links



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