Background giants in the field of the globular cluster M22: Kinematics of the galactic bulge

Dante Minniti, James Liebert, Edward W. Olszewski, Simon D.M. White

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

5 Citas (Scopus)

Resumen

We report radial velocities, metallicities, and near-IR photometry for about 100 giants in the field of the globular cluster M22, at l,b=(9.9°,-7.6°). Most of them are bulge giants, non-members of the cluster from proper motions. Dividing the sample according to metallicity, we find that the giants more metal-poor than [Fe/H]≈-1 have halo-like kinematics, while the more metal-rich giants have higher rotation and smaller velocity dispersion, which we identify with the bulge. Such dependences of kinematics on metal abundance (which may be due to a mix of populations) are predicted by dissipational collapse models of formation for the inner Galaxy. The 11 M giants in the field follow bulge rather than halo kinematics.

Idioma originalInglés
Páginas (desde-hasta)590-600
Número de páginas11
PublicaciónAstronomical Journal
Volumen112
N.º2
DOI
EstadoPublicada - ago 1996

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

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