NGC 1566
NGC 1566, sometimes known as the Spanish Dancer,[3][4] is an intermediate spiral galaxy in the constellation Dorado. It is the dominant and brightest member[5] of the Dorado Group,[6][7] being among the brightest Seyfert galaxies in the sky.[5] Absolute luminosity is 3.7×1010 L☉,[8] and is calculated to contain 1.4×1010 M☉ of H I.[8]
NGC 1566 | |
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A close-up image of NGC 1566 taken by the Hubble’s Wide Field Camera 3. | |
Observation data (J2000 epoch) | |
Constellation | Dorado |
Right ascension | 4h 20m .4s[1] |
Declination | −54° 56′ 16″[1] |
Redshift | 0.005017[1] |
Helio radial velocity | 1504 ± 2 km/s[1] |
Distance | 38.4 ± 18.6 Mly (11.8 ± 5.7 Mpc)[2] |
Apparent magnitude (V) | 10.3[1] |
Characteristics | |
Type | SAB(rs)bc[1] |
Apparent size (V) | 8′.3 × 6′.6[1] |
Other designations | |
PGC 14897[1] |
SN 2010el
On June 19, 2010, Berto Monard from South Africa detected a magnitude 16 supernova 13" west and 22" south of the center of NGC 1566 at coordinates 04 19 58.83 -54 56 38.5.[9]
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gollark: ++Delete <@319753218592866315> (killing kittenenes)
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References
- "NASA/IPAC Extragalactic Database", Results for NGC 1566, retrieved 2007-04-01
- "Distance Results for NGC 1566". NASA/IPAC Extragalactic Database. Retrieved 2010-06-21.
- "Spanish Dancer Galaxy - NGC 1566 - Billions and Billions.com". billionsandbillions.com. Retrieved 2015-10-13.
- "NGC 1566 Spanish Dancer Galaxy in Dorado | Amazing Sky Astrophotography by Alan Dyer". amazingsky.photoshelter.com. Retrieved 2015-10-13.
- de Vaucouleurs, Gérard (April 1, 1973), "Southern Galaxies.VI. Luminosity Distribution in the Seyfert Galaxy NGC 1566", Astrophysical Journal, 181: 31–50, Bibcode:1973ApJ...181...31D, doi:10.1086/152028
- Huchra, John Peter; Geller, Margaret J. (June 15, 1982), "Groups of galaxies. I - Nearby groups", Astrophysical Journal, 257 (Part 1): 423–437, Bibcode:1982ApJ...257..423H, doi:10.1086/160000
- Firth, P.; Evstigneeva, E. A.; Jones, J. B.; Drinkwater, M. J.; et al. (November 2006), "Kinematics, substructure and luminosity-weighted dynamics of six nearby galaxy groups", Monthly Notices of the Royal Astronomical Society, 372 (4): 1856–1868, arXiv:astro-ph/0608584, Bibcode:2006MNRAS.372.1856F, doi:10.1111/j.1365-2966.2006.10993.x
- Virginia A. Kilborn; Bärbel S. Koribalski; Duncan A. Forbes; David G. Barnes; et al. (January 2005), "A Wide-Field Hi Study of the NGC 1566 Group", Monthly Notices of the Royal Astronomical Society, 356 (1): 77–88, arXiv:astro-ph/0409743, Bibcode:2005MNRAS.356...77K, doi:10.1111/j.1365-2966.2004.08450.x
- David Bishop. "Latest Supernovae". supernovae.net (International Supernovae Network). Retrieved 2010-06-21.
External links
Wikimedia Commons has media related to NGC 1566. |
- Spitzer Space Telescope page on NGC 1566
- Discovery image of SN 2010el (2010-06-19; The star to the left of the core of the galaxy is magnitude 12.3)
- NGC 1566 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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