T Tauri winds and their relationship to molecular outflows.

Details T Tauri winds and their relationship to molecular outflows. T Tauri winds and their relationship to molecular outflows.

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esoc...33..365n&link_type=abstract

ESO Workshop on Low Mass Star Formation and Pre-Main Sequence Objects, p. 365 - 383

Physics

15

Pre-Main-Sequence Stars: Stellar Winds, Pre-Main-Sequence Stars: Mass Loss, Pre-Main-Sequence Stars: Carbon Monoxide

Scientific paper

The properties of winds from low-mass, pre-main sequence stars and their relationship to the CO outflows often associated with them, are discussed. Most pre-main sequence stars have winds with relatively low rates of mass-loss (M˙ ⪉ 10-8Msunyr-1). However, in a significant number of cases (T Tauri stars with P Cygni profiles in Na I lines), M˙ is higher. In these cases, the innermost region of the wind is cool (Tg ⪉ 7000K) and mostly neutral. Forbidden line emission and radio continuum emission are likely to be secondary indicators of the winds, possibly formed in shock regions.

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