Oh as a Signpost of Accretion in T Tauri Stars

Details Oh as a Signpost of Accretion in T Tauri Stars Oh as a Signpost of Accretion in T Tauri Stars

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.5880h&link_type=abstract

HST Proposal ID #5880

Physics

Hst Proposal Id #5880 Cool Stars

Scientific paper

The H_2O in the interstellar material moving inward in the accretion disk around a T Tauri star, if it is similar to the material in cometary nuclei, will be dissociated by the ultraviolet radiation of the star. A major product is OH, which is detectable in emission by resonance scattering of the 0--0 band near 3100 Angstrom. We propose to examine T Tau and RU Lup for this phenomenon.

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