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Properties of hot stars in the Wolf--Rayet galaxy NGC 5253 from ISO-SWS spectroscopy
Authors:Paul A. Crowther   S. C. Beck  Allan J. Willis  Peter S. Conti  Patrick W. Morris   Ralph S. Sutherland
Affiliation:Department of Physics &Astronomy, University College London, Gower Street, London WC1E 6BT; School of Physics &Astronomy of the Raymond &Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Ramat Aviv, Israel; JILA, University of Colorado, Boulder, CO 80309, USA; ISO Science Operation Centre, Astrophysics Division, ESA, PO Box 50727, E-28080 Villafranca, Madrid, Spain; SRON, Sorbonnelaan 2, CA 3584 Utrecht, the Netherlands; Mount Stromlo and Siding Spring Observatories, Australian National University, Canberra, ACT 0200, Australia
Abstract:
Keywords:stars: Wolf-Rayet    galaxies: individual: NGC 5253    galaxies: starburst    galaxies: stellar content    infrared: galaxies
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