Protoplanetary Disks around TTauri Stars in Taurus-Auriga Clouds

Details Protoplanetary Disks around TTauri Stars in Taurus-Auriga Clouds Protoplanetary Disks around TTauri Stars in Taurus-Auriga Clouds

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pcim.conf..265d&link_type=abstract

The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium, held in Zermatt, Septemb

Physics

Scientific paper

Due to technological improvements, in about five years, mm arrays have completely changed our knowledge of protoplanetary disks. In particular, sub-arcsecond images of the dust and gas distribution allow for the first time accurate modelling of their properties. At IRAM, we intensively used the Plateau de Bure interferometer to investigate the physical properties of the circumstellar disks found around low-mass TTauri stars in the Taurus-Auriga clouds. Studies of the circumbinary disk of GG Tau and of the circumstellar disk of DM Tau are among the best examples showing the fast evolution and potential of mm interferometers. They can easily be extrapolated to the needs for the future mm arrays.

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