Astrophysics Research Institute / Space Telescope Science Institute / Herzberg Institute of Astrophysics / Egerton Wharf / Liverpool John Moores University / National Optical Astronomy Observatory / /
IndustryTerm
power-law distribution / metal-poor clusters / satellite trails / metal-rich clusters / power-law indices / metal-rich population / power-law fits / gas density / gas-rich material / gas-rich spirals / gas-rich galaxies / metal-poor cluster population / globular cluster systems / molecular gas / metal-poor population / shocked interstellar gas / metal / dynamical and chemical assembly histories / satellite start / gas-rich satellite disk galaxy / metal-rich younger population / metal-rich peak / power-law fit / metal-poor globular cluster population / power law / younger and more metal-rich population / metal-poor / metal-rich subpopulation / /
NaturalFeature
Wide Field Channel / /
Organization
Liverpool John Moores University / Association of Universities for Research / National Science Foundation / International Monetary Fund / Space Telescope Science Institute / KMM / Herzberg Institute of Astrophysics / National Aeronautics and Space Administration / American Astronomical Society / Astrophysics Research Institute / /
Person
Vega / /
Position
General / /
Product
Galaxy / /
ProvinceOrState
Alabama / Maryland / Victoria / California / /
PublishedMedium
The Astronomical Journal / /
RadioStation
SHELL GALAXY AM 0139 / POPULATIONS IN AM 0139 / PHOTOMETRY AM 0139 / AM 0139 / IN AM 0139 / FUNCTION OF AM 0139 / /
The Astronomical Journal, 134:1729–1739, 2007 November # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. EVIDENCE FOR THREE SUBPOPULATIONS OF GLOBULAR CLUSTERS IN THE EARLY-TYPE POSTSTAR