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Lee, Hyun-chul - Department of Physics and Astronomy, Washington State University
ON THE AGE AND METALLICITY ESTIMATION OF SPIRAL GALAXIES USING OPTICAL AND NEAR-INFRARED PHOTOMETRY
1999 Macmillan Magazines Ltd derive the initial luminosity L from L L*=f giant
HORIZONTAL-BRANCH MORPHOLOGY AND THE PHOTOMETRIC EVOLUTION OF OLD STELLAR POPULATIONS
Effects of Alpha-Element Enhancement and the Thermally Pulsing-Asymptotic Giant Branch on Surface Brightness
Theoretical Realization of Near-Infrared Photometry of
GLOBULAR CLUSTER AND GALAXY FORMATION: M31, THE MILKY WAY, AND IMPLICATIONS FOR GLOBULAR CLUSTER SYSTEMS OF SPIRAL GALAXIES1
arXiv:0905.1947v1[astro-ph.GA]13May2009 Comparison of Alpha-Element Enhanced Simple Stellar
The Astrophysical Journal, 694:902923, 2009 April 1 doi:10.1088/0004-637X/694/2/902 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
STELLAR POPULATION MODELS AND INDIVIDUAL ELEMENT ABUNDANCES. I. SENSITIVITY OF STELLAR EVOLUTION MODELS
-ENHANCED INTEGRATED LICK/IDS SPECTRAL INDICES AND MILKY WAY AND M31 GLOBULAR CLUSTERS AND EARLY-TYPE GALAXIES
We study these effects at ages covering 0.1 to 13 Gyr and metallicities of Z=0.0003 to 0.04 using the Teramo group's isochrones, BaSTI, in order to investigate the calibration zero-point.
THE ASTRONOMICAL JOURNAL, 120:9981005, 2000 August 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
arXiv:0905.2407v1[astro-ph.GA]14May2009 To appear in Astronomical Journal
arXiv:astro-ph/0604590v127Apr2006 Draft version April 15, 2009
arXiv:astro-ph/0210178v18Oct2002 Blue Horizontal-Branch Stars
