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NGC 6638

From Wikipedia, the free encyclopedia
Globular cluster in the constellation Sagittarius
NGC 6638
Observation data (J2000epoch)
ClassVI
ConstellationSagittarius
Right ascension18h 30m 56.2s
Declination−25° 29′ 45″
Distance31.3 ± 1.6 kly (9.6 ± 0.5 kpc)[1]
Apparent magnitude (V)9.5
Apparent dimensions (V)2′
Physical characteristics
Mass1.89×105[1] M
Other designationsGCl 95, C 1827-255[2]
See also:Globular cluster,List of globular clusters

NGC 6638 is aglobular cluster in the constellationSagittarius. It is magnitude 9.5 and diameter 2 arc minutes, class VI. It is a half degree east ofLambda Sagittarii. It is a member of the Milky Way.[3]

The globular cluster was discovered in 1784 by the astronomerWilliam Herschel with his 18.7-inch telescope and the discovery was later entered in theNew General Catalogue.

References

[edit]
  1. ^abOliveira, R. A. P.; Ortolani, S.; Barbuy, B.; Kerber, L. O.; Maia, F. F. S.; Bica, E.; Cassisi, S.; Souza, S. O.; Pérez-Villegas, A. (2022). "Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters".Astronomy & Astrophysics.657: A123.arXiv:2110.13943.Bibcode:2022A&A...657A.123O.doi:10.1051/0004-6361/202141596.S2CID 239998638.
  2. ^"NGC 6638".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-02-11.
  3. ^Harris, W.E. (1996)."A Catalog of Parameters for Globular Clusters in the Milky Way".The Astronomical Journal.112: 1487.Bibcode:1996AJ....112.1487H.doi:10.1086/118116.
  • Robert Burnham Jr.,Burnham's Celestial Handbook: An observer's guide to the universe beyond the solar system, vol 3, p. 1557

External links

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