Astronomy:NGC 5634

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NGC 5634
File:250px
The globular cluster NGC 5634 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ClassIV [1]
ConstellationVirgo
Right ascension 14h 29m 37.28s[2]
Declination−05° 58′ 35.1″[2]
Distance81.9 ± 3.8 kly (25.12 ± 1.16 kpc)[3]
Apparent magnitude (V)10.05[2]
Physical characteristics
Radius2.45' x 2.45'[4]
Metallicity[Fe/H] = −1.8 ± 0.1[3] dex
Estimated age12.8 ± 0.3 Gyr[3]
Other designationsGCl 28, GCRV 8456[2]
See also: Globular cluster, List of globular clusters

NGC 5634 is a globular cluster in the constellation Virgo, located about 82,000 light years (25.12 kiloparsecs) from Earth.[2] NGC 5634 has an apparent magnitude of about 10[2] and a diameter of 4 or 5 arcminutes.[4] Its Shapley–Sawyer Concentration Class is IV,[1] meaning the cluster shows intermediate rich concentrations. The star near the upper right is the eleventh-magnitude UCAC2 29844847. There is also a bright orange giant, HD 127119, about 1.3 arcminutes away from the cluster.

The origin of NGC 5634 is somewhat unclear; it was once thought to be a likely member of the Sagittarius Dwarf Spheroidal Galaxy,[4] but it may be associated with Gaia-Sausage-Enceladus or the Helmi stream instead.[3]

References

  1. 1.0 1.1 Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin 849 (849): 11–14, Bibcode1927BHarO.849...11S. 
  2. 2.0 2.1 2.2 2.3 2.4 2.5 "NGC 5634". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+5634. 
  3. 3.0 3.1 3.2 3.3 Wang 王, Shouzhi 守智; Nie 聂, Jundan 俊丹; Jiang 姜, Biwei 碧沩; Tian 田, Hao 浩.; Liu 刘, Chao 超.; Zhang 张, Ying-Hua 颖华 (2025). "The Structural and Kinematical Properties of NGC 5634, a Globular Cluster Associated with the Sagittarius Dwarf Galaxy?". The Astrophysical Journal 988 (1): 39. doi:10.3847/1538-4357/ade0b6. Bibcode2025ApJ...988...39W. 
  4. 4.0 4.1 4.2 "spider.seds.org NGC 5634". http://spider.seds.org/spider/MWGC/n5634.html. 

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