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Infrared stellar populations in the central parts of the Milky Way galaxy
Authors:Jacco Th. van Loon  G. F. Gilmore  A. Omont  J. A. D. L. Blommaert  I. S. Glass  M. Messineo  F. Schuller  M. Schultheis  I. Yamamura   H. S. Zhao
Affiliation:Astrophysics Group, School of Chemistry &Physics, Keele University, Staffordshire ST5 5BG;Institute of Astronomy, Madingley Road, Cambridge CB3 0HA;Institut d'Astrophysique de Paris, CNRS, 98 bis Boulevard Arago, F-75014 Paris, France;Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, B-3001 Leuven, Belgium;South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa;Leiden Observatory, PO Box 9513, NL-2300 RA Leiden, the Netherlands;Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229, Japan
Abstract:
Keywords:stars: AGB and post-AGB    dust, extinction    Galaxy: evolution    Galaxy: stellar content    Galaxy: structure    infrared: stars
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