Debris Discs Around Stars: The 2004 ISO Legacy

Details Debris Discs Around Stars: The 2004 ISO Legacy Debris Discs Around Stars: The 2004 ISO Legacy

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ssrv..119..201d&link_type=abstract

Space Science Reviews, Volume 119, Issue 1-4, pp. 201-214

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Scientific paper

Debris discs around stars were first discovered by the Infrared Astronomical Satellite (IRAS) in 1983. For the first time material orbiting another star than the Sun, but distinct from a circumstellar envelope, was observed through its far infrared emission. This major discovery motivated astronomers to investigate those discs by further analyzing the IRAS data, using ground-based telescopes for the hunting of exoplanets, developing several projects using the Infrared Space Observatory (ISO), and now exploiting the ISO Data Archive (IDA). This review presents the main ISO results, statistical as well as individual, on debris discs in orbit around pre-main-sequence and main-sequence stars.

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