NGC 4372

NGC 4372
Observation data (J2000 epoch)
Class XII[1]
Constellation Musca
Right ascension 12h 26m 00s
Declination −72° 40
Distance 18.9 kly (5.8 kpc)[2]
Apparent magnitude (V) 7.8
Physical characteristics
Mass 3.29×105[2] M
Metallicity \begin{smallmatrix}\left[{Fe}/{H}\right]\end{smallmatrix} = –1.88[3] dex
Estimated age 12.54 Gyr[3]
Other designations Caldwell 108

NGC 4372 is a globular cluster in the southern constellation of Musca.

References

  1. Shapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters", Harvard College Observatory Bulletin (849): 11–14, Bibcode:1927BHarO.849...11S.
  2. 1 2 Boyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters", The Astrophysical Journal 742 (1): 51, arXiv:1108.4402, Bibcode:2011ApJ...742...51B, doi:10.1088/0004-637X/742/1/51.
  3. 1 2 Forbes, Duncan A.; Bridges, Terry (May 2010), "Accreted versus in situ Milky Way globular clusters", Monthly Notices of the Royal Astronomical Society 404 (3): 1203–1214, arXiv:1001.4289, Bibcode:2010MNRAS.404.1203F, doi:10.1111/j.1365-2966.2010.16373.x.

External links

Coordinates: 12h 26m 00s, −72° 40′ 00″

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