The Globular Cluster System of the Virgo Giant Elliptical Galaxy NGC 4636: I. Subaru/FOCAS Spectroscopy and Database
Hong Soo Park (1), Myung Gyoon Lee (1), Ho Seong Hwang (1,2), Nobuo, Arimoto (3), Naoyuki Tamura (4), Masato Onodera (2) ((1) Seoul National, Univ.,(2) CEA, Laboratoire AIM, (3) National Astronomical Observatory of, Japan, (4) Subaru Telescope)

TL;DR
This study spectroscopically analyzed 122 globular clusters in NGC 4636, measuring their velocities and dispersions, and compiled a comprehensive catalog to understand the galaxy's globular cluster system.
Contribution
It provides new spectroscopic velocity measurements for GCs in NGC 4636 and creates a master catalog combining previous data for detailed kinematic analysis.
Findings
Velocity dispersion of GCs is approximately 225 km/s.
Blue GCs have a slightly higher velocity dispersion than red GCs.
The mean velocity of GCs aligns with the galaxy nucleus velocity.
Abstract
We present a spectroscopic study of the globular clusters (GCs) in the giant elliptical galaxy NGC 4636 in the Virgo cluster. We selected target GC candidates using the Washington photometry derived from the deep CCD images taken at the KPNO 4m. Then we obtained the spectra of 164 target objects in the field of NGC 4636 using the Multi-Object Spectroscopy (MOS) mode of Faint Object Camera and Spectrograph (FOCAS) on the SUBARU 8.2m Telescope. We have measured the velocities for 122 objects: 105 GCs in NGC 4636, the nucleus of NGC 4636, 11 foreground stars, 2 background galaxies, and 3 probable intracluster GCs in the Virgo cluster. The GCs in NGC 4636 are located in the projected galactocentric radius within 10arcmin (corresponding to 43 kpc). The measured velocities for the GCs range from 300km/s to 1600km/s, with a mean value of 932_{-22}^{+25} km/s, which is in good agreement with…
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