The Stellar Content Near the Galactic Center

Abstract

High angular resolution J, H, K, and L' images are used to investigate the stellar content within 6 arcsec of SgrA*. The data, which are complete to K ~ 16, are the deepest multicolor observations of the region published to date.

34 pages, including 12 figures

Cited by in corpus (19)

• The Stellar Cusp Around the Supermassive Black Hole in the Galactic Center
• Stellar Processes Near the Massive Black Hole in the Galactic Center
• Jet directions in Seyfert galaxies
• Really Cool Stars and the Star Formation History at the Galactic Center
• Evidence for a Long-Standing Top-Heavy IMF in the Central Parsec of the Galaxy
• The distribution of stars near the super-massive black hole in the Galactic Center
• Near-Infrared Microlensing of Stars by the Super-Massive Black Hole in the Galactic Center
• L- and M-band imaging observations of the Galactic Center region
• Modern optical astronomy: technology and impact of interferometry
• High Angular Resolution JHK Imaging of the Centers of the Metal-Poor Globular Clusters NGC5272 (M3), NGC6205 (M13), NGC6287, and NGC6341 (M92)
• Radial Velocities of Stars in the Galactic Center
• Enhanced Microlensing by Stars Around the Black Hole in the Galactic Center
• Deep ALTAIR + NIRI Imaging of the Disk and Bulge of M31
• Near-Infrared Adaptive Optics Imaging of the Central Regions of Nearby Sc Galaxies: I. M33
• The Central Regions of M81
• The Near-Infrared Photometric Properties of Bright Giants in the Central Regions of the Galactic Bulge
• The Central Regions of M31 in the 3 - 5 micron Wavelength Region
• The Near-Infrared Spectrum of the Nuclear Star Cluster: Looking Below the Tip of the Iceberg and Comparisons with Extragalactic Nuclei
• Composition of the galactic center star cluster: Population analysis from adaptive optics narrow band spectral energy distributions