The circumstellar environment of the GG Tauri multiple system

Details The circumstellar environment of the GG Tauri multiple system The circumstellar environment of the GG Tauri multiple system

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...36..281k&link_type=abstract

In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36

Physics

Accretion Disks, Binary Stars, Pre-Main Sequence Stars, Stellar Envelopes, Stellar Systems, Celestial Mechanics, Interstellar Gas

Scientific paper

We present (C-13)O(2 - 1) aperture synthesis maps of the circumstellar environment of GG Tau, a very young binary system. An extensive, approximately edge-on, gaseous disk in near-Keplerian rotation is detected. The disk emission is severely affected by the presence of GG Tau/c, a second binary system at a projected distance of 1500 AU from GG Tau and apparently in the plane of the disk.

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