Deep Near‐Infrared Array Photometry of Globular Clusters. VI. NGC 288
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/475/i=2/a=584/pdf
Reference55 articles.
1. The main sequence of the globular cluster NGC 288
2. The properties of the disk system of globular clusters
3. Luminosity functions for post-turnoff stars in globular clusters. I - NGC 288
4. Oxygen-enhanced models for globular cluster stars. II - Isochrones and luminosity functions
5. The age of the globular cluster NGC 288, the formation of the Galactic halo, and the second parameter
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2. Halo globular clusters observed with AAOmega: dark matter content, metallicity and tidal heating;Monthly Notices of the Royal Astronomical Society;2010-05-25
3. Red giant branch in near-infrared colour-magnitude diagrams - I. Calibration of photometric indices;Monthly Notices of the Royal Astronomical Society;2004-07
4. A Near-Infrared Photometric Survey of Metal-poor Inner Spheroid Globular Clusters and Nearby Bulge Fields;The Astronomical Journal;2000-10
5. High Angular Resolution [ITAL]JHK[/ITAL] Imaging of the Centers of the Metal-poor Globular Clusters NGC 5272 (M3), NGC 6205 (M13), NGC 6287, and NGC 6341 (M92);The Astronomical Journal;1999-03
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