ISO Observations of Pre-Main Sequence and Vega-type Stars

Details ISO Observations of Pre-Main Sequence and Vega-type Stars ISO Observations of Pre-Main Sequence and Vega-type Stars

2000-05-03

arxiv.org/abs/astro-ph/0005060v1

Astronomy and Astrophysics

Astrophysics

12 pages, 2 figures, invited review to appear in proc. ``Disks, Planetesimals and Planets'', eds. F. Garz\'on et al

Scientific paper

I present an overview of the results obtained by the Infrared Space Observatory (ISO) on circumstellar material in pre-main sequence (PMS) stars. Results obtained for embedded YSOs, Herbig Ae/Be systems and T Tauri stars are reviewed and their connection to the disks around Vega-type systems is discussed. Although the gas contents of the PMS environment will also be discussed briefly, this review will mainly focus on the composition, mineralogy and evolution of dust in these systems, and the results will be compared to those found in other classes of objects, including solar system comets.

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