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ISO observations of obscured Asymptotic Giant Branch stars in the Large Magellanic Cloud.pdf

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ISO observations of obscured Asymptotic Giant Branch stars in the Large Magellanic Cloud

a r X i v : a s t r o - p h / 9 9 0 4 3 5 3 v 1 2 6 A p r 1 9 9 9 AA manuscript no. (will be inserted by hand later) Your thesaurus codes are: 06(08.03.1; 08.03.4; 08.13.2; 08.16.4; 11.13.1; 13.09.6) ASTRONOMY AND ASTROPHYSICS ISO observations of obscured Asymptotic Giant Branch stars in the Large Magellanic Cloud? Norman R. Trams1, Jacco Th. van Loon2, L.B.F.M. Waters2,3, Albert A. Zijlstra4, Cecile Loup5, Patricia A. Whitelock6, M.A.T. Groenewegen7, Joris A.D.L. Blommaert8, Ralf Siebenmorgen8, A. Heske8 and Michael W. Feast9 1 Integral Science Operations Centre, Astrophysics Div., Science Dep., ESTEC, P.O.Box 299, NL-2200 AG Noordwijk, The Netherlands 2 Astronomical Institute, University of Amsterdam, Kruislaan 403, NL-1098 SJ Amsterdam, The Netherlands 3 Space Research Organization Netherlands, Landleven 12, NL-9700 AV Groningen, The Netherlands 4 University of Manchester Institute of Science and Technology, P.O.Box 88, Manchester M60 1QD, United Kingdom 5 Institut d’Astrophysique de Paris, 98bis Boulevard Arago, F-75014 Paris, France 6 South African Astronomical Observatory, P.O.Box 9, 7935 Observatory, South Africa 7 Max-Planck Institut fu?r Astrophysik, Karl-Schwarzschild Stra?e 1, D-85740 Garching bei Mu?nchen, Germany 8 ISO Data Centre, Astrophysics Division, Science Department of ESA, Villafranca del Castillo, P.O.Box 50727, E-28080 Madrid, Spain 9 Astronomy Department, University of Cape Town, 7700 Rondebosch, South Africa Received date; accepted date Abstract. We present ISO photometric and spectro- scopic observations of a sample of 57 bright Asymptotic Giant Branch stars and red supergiants in the Large Mag- ellanic Cloud, selected on the basis of IRAS colours indica- tive of high mass-loss rates. PHOT-P and PHOT-C pho- tometry at 12, 25 and 60 μm and CAM photometry at 12 μm are used in combination with quasi-simultaneous ground-based near-IR photometry to construct colour- colour diagrams for all stars in our sample. PHOT-S and CAM-CVF spectra in