POSTER PAPER 7.04

ISOPHOT Observations of a Selected Sample of Flare Stars
G. Leto, M. Rodono, I. Pagano, G. Marino

Institute: INAF - Catania Astrophysical Observatory, Italy
Institute: Department of Physics and Astronomy of Catania University, Italy
Institute: INAF- CNAA, Centro Galileo Galilei, Spain
Contact Email: gle@ct.astro.it

Abstract: A selected sample of UV Cet-type stars were photometrically observed by ISOPHOT on ISO to trace their spectral energy distribution in the 2-200 micrometers spectral range. We report on our data analysis which confirms the presence of an IR excess for some of the observed sources, as already suggested by IRAS data. The nature of this IR excess is under investigation.

ISOPHOT Observations of a Selected Sample of Flare Stars [PDF - Type 1 fonts]

ISOPHOT Observations of a Selected Sample of Flare Stars [PS]

Index Keywords: EV Lac

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Manuscript submitted: 2001-Sep-03
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown, G. M. Harper, & T. R. Ayres. Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems, & The Sun,
© 2003 University of Colorado.