Circumstellar dust around main-sequence stars: what can we learn from the ISOPHOT archive?

Details Circumstellar dust around main-sequence stars: what can we learn from the ISOPHOT archive? Circumstellar dust around main-sequence stars: what can we learn from the ISOPHOT archive?

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..129a&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Circumstellar dust around main-sequence stars, the Vega phenomenon, was the topic of a number of ISOPHOT key projects. The results of these projects were published in separate papers without combining their data. In this contribution we discuss the possible merrits of collecting and re-analysing all normal star observations from the ISOPHOT archive, and present preliminary results extracted from a collection of minimap observations performed with the ISOPHOT C100 camera at 60μm.

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