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NGC 2244

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This is an old revision of this page, as edited by Headbomb (talk | contribs) at 02:56, 30 July 2015 (Cleanup for Book:Caldwell catalogue, replaced: }}, {{doi|10.1051/0004-6361/201117458}} → }} | doi = 10.1051/0004-6361/201117458 using AWB). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 2244
An infrared Spitzer Space Telescope (SIRT) image of NGC 2244.
Credit: SIRT/NASA
Observation data (J2000 epoch)
Right ascension6h 31m 54s[1]
Declination+4° 56′[1]
Distance5.2 kly
Apparent magnitude (V)4.8[1]
Apparent dimensions (V)24′
Physical characteristics
Other designationsCaldwell 50
Associations
ConstellationMonoceros
See also: Open cluster, List of open clusters

NGC 2244 (also known as Caldwell 50) is an open cluster in the Rosette Nebula, which is located in the constellation Monoceros. This cluster has several O-type stars, super hot stars that generate large amounts of radiation and stellar wind.

The age of this cluster has been estimated to be less than 5 million years and its two brightest stars are HD 46223 of spectral class O4V, 400,000 times brighter than the Sun, and approximately 50 times more massive, and HD 46150, whose spectral type is O5V, has a luminosity 450,000 time larger than that of our star, and is up to 60 times more massive, but it may actually be a double star.[2]

References

  1. ^ a b c "SIMBAD Astronomical Database". Results for NGC 2244. Retrieved 2007-04-20.
  2. ^ A quantitative study of O stars in NGC 2244 and the Monoceros OB2 association, Martins, F.; Mahy, L.; Hillier, D. J.; Rauw, G., Astronomy and Astrophysics 538, pp. A39, Bibcode:2012A&A...538A..39M, doi:10.1051/0004-6361/201117458.
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