Pre-main sequence disks

Details Pre-main sequence disks Pre-main sequence disks

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..270...45d&link_type=abstract

Computational Star Formation, Proceedings of the International Astronomical Union, IAU Symposium, Volume 270, p. 45-48

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Stars: Formation, Circumstellar Matter, Stars: Pre-Main Sequence

Scientific paper

In this contribution, I briefly review our empirical knowledge of disks around <~2Msolar pre-main sequence (T Tauri) stars, focusing first on the dichotomic question of their frequency before moving on to some more detailed disk properties (overall orientation, total mass, outer radius). Finally, I conclude with a brief discussion of disks around embedded protostars, which will play in the next few years a major role in testing star formation theory and simulations.

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