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NGC 6221

Coordinates:Sky map16h52m46.1s,+-59° 13′ 07″
From Wikipedia, the free encyclopedia
NGC6221
NGC 6221 as seen through theHubble Space Telescope
Observation data (J2000epoch)
ConstellationAra
Right ascension16h52m46.1s[1]
Declination−59° 13′ 07″[1]
Redshift0.004999±0.000017[1]
Heliocentric radial velocity1499±5 km/s[1]
Galactocentric velocity1390±7 km/s[1]
Apparent magnitude(V)9.28[1]
Absolute magnitude(V)−20.97[1]
Characteristics
TypeSB(s)bc[1]
Size70,000light years
Apparent size(V)3.5× 2.5[1]
Other designations
ESO138-3, AM 1648-590,IRAS16484-5908 andPGC59175
References:NASA/IPAC extragalactic datatbase,http://spider.seds.org/

NGC 6221(also known asPGC59175) is abarred spiral galaxylocated in the constellationAra.In de Vaucouleurs'galaxy morphological classification scheme,it is classified as SB(s)bc[1]and was discovered by British astronomerJohn Herschelon 3 May 1835.[2]NGC 6221 is located at about 69 millionlight yearsfrom Earth.[1][3]

In 1990, atype Ib/Icsupernovawas detected within NGC 6221, and was designated SN 1990W.[4]

Galaxy group information

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NGC 6221 is part ofgalaxy groupNGC 6221/15, which includesspiral galaxyNGC 6215and threedwarf galaxies.Interactions between NGC 6221 and NGC 6215 form adouble-stranded bridgeofneutral hydrogen gasover a projected distance of 100kpc;Dwarf 3 of the three dwarf galaxies may have formed from the bridging gas.[5]

See also

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References

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  1. ^abcdefghijk"Object No. 1 - NGC 6221".NASA/IPAC extragalactic database.NASA/IPAC.Retrieved3 October2015.
  2. ^"NGC 6221 (= PGC 59175)".cseligman.Retrieved3 October2015.
  3. ^"Revised NGC Data for NGC 6221".Seds.Retrieved3 October2015.
  4. ^"SN 1990W".SIMBAD.Centre de données astronomiques de Strasbourg.Retrieved2021-03-19.
  5. ^Koribalski, Bärbel; Dickey, John M. (2005)."Neutral Hydrogen Gas in Interacting Galaxies: The NGC 6221 / 6215 galaxy group".Monthly Notices of the Royal Astronomical Society.348(4): 202–210.arXiv:astro-ph/0501190.Bibcode:2004MNRAS.348.1255K.doi:10.1111/j.1365-2966.2004.07444.x.Retrieved17 December2015.
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