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NGC 1566

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NGC 1566
A mid-infrared image of NGC 1566 taken by the Spitzer Space Telescope (SST).
Observation data (J2000 epoch)
ConstellationDorado
Right ascension4h 20m .4s[1]
Declination−54° 56′ 16″[1]
Redshift1504 ± 2 km/s[1]
Apparent magnitude (V)10.3[1]
Characteristics
TypeSAB(rs)bc[1]
Apparent size (V)8′.3 × 6′.6[1]
Other designations
PGC 14897[1]

NGC 1566 is an intermediate spiral galaxy in the constellation Dorado. It is the dominant[2] member of the Dorado Group and also its brightest member.[3][4] It is the second brightest Seyfert galaxy after NGC 1068.[2] Its absolute luminosity is 3.7×1010 L.[5] It contains 1.4×1010 M of H I.[5]

References

  1. ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 1566. Retrieved 2007-04-01.
  2. ^ a b de Vaucouleurs, Gérard (April 1 1973), "Southern Galaxies.VI. Luminosity Distribution in the Seyfert Galaxy NGC 1566", Astrophysical Journal, 181: 31–50, doi:10.1086/152028 {{citation}}: Check date values in: |date= (help)CS1 maint: date and year (link)
  3. ^ Huchra, John Peter; Geller, Margaret J. (June 15 1982), "Groups of galaxies. I - Nearby groups", Astrophysical Journal, 257 (Part 1): 423–437, doi:10.1086/160000 {{citation}}: Check date values in: |date= (help)CS1 maint: date and year (link)
  4. ^ Firth, P.; Evstigneeva, E. A.; Jones, J. B.; Drinkwater, M. J.; Phillipps, S.; Gregg, M. D. (November 2006), "Kinematics, substructure and luminosity-weighted dynamics of six nearby galaxy groups", Monthly Notices of the Royal Astronomical Society, 372 (4): 1856–1868, doi:10.1111/j.1365-2966.2006.10993.x{{citation}}: CS1 maint: date and year (link) CS1 maint: multiple names: authors list (link)
  5. ^ a b Virginia A. Kilborn; Bärbel S. Koribalski; Duncan A. Forbes; David G. Barnes; Ruth C. Musgrave (January 2005), "A Wide-Field Hi Study of the NGC 1566 Group", Monthly Notices of the Royal Astronomical Society, 356 (1): 77–88, doi:10.1111/j.1365-2966.2004.08450.x{{citation}}: CS1 maint: date and year (link) CS1 maint: multiple names: authors list (link)