ISOPHOT Observations of a Selected Sample of Flare Stars

Details ISOPHOT Observations of a Selected Sample of Flare Stars ISOPHOT Observations of a Selected Sample of Flare Stars

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..970l&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

Ev Lac

Scientific paper

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 μ m 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.

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