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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
Institution: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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