The Globular Cluster System of M60 (NGC 4649). I. CFHT MOS Spectroscopy and Database
arXiv:0709.4308 · doi:10.1086/522956
Abstract
We present the measurement of radial velocities for globular clusters in M60, giant elliptical galaxy in the Virgo cluster. Target globular cluster candidates were selected using the Washington photometry based on the deep $16\arcmin \times 16\arcmin$ images taken at the KPNO 4m and using the photometry derived from the HST/WFPC2 archive images. The spectra of the target objects were obtained using the Multi-Object Spectrograph (MOS) at the Canada-France-Hawaii Telescope (CFHT). We have measured the radial velocity for 111 objects in the field of M60: 93 globular clusters (72 blue globular clusters with and 21 red globular clusters with ), 11 foreground stars, 6 small galaxies, and the nucleus of M60. The measured velocities of the 93 globular clusters range from km s to km s, with a mean value of km s, which is in good agreement with the velocity of the nucleus of M60 ( km s). Combining our results with data in the literature, we present a master catalog of radial velocities for 121 globular clusters in M60. The velocity dispersion of the globular clusters in the master catalog is found to be km s for the entire sample, km s for 83 blue globular clusters, and km s for 38 red globular clusters.
29 pages, 8 figures. To appear in ApJ
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- Spatial Structures In the Globular Cluster Distribution of the Ten Brightest Virgo Galaxies
- Resolving the Discrepancy of Distance to M60, a Giant Elliptical Galaxy in Virgo
- Nonlinear Color-Metallicity Relations of Globular Clusters. IX. Different Radial Number Density Profiles between Blue and Red Clusters
- Nonlinear Color-Metallicity Relations of Globular Clusters. X. Subaru/FOCAS Multi-object Spectroscopy of M87 Globular Clusters
- The total mass of the early-type galaxy NGC 4649 (M60)