Possible detection of a high-velocity neutral wind in T Tauri

Details Possible detection of a high-velocity neutral wind in T Tauri Possible detection of a high-velocity neutral wind in T Tauri

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...394l..57r&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 394, no. 2, Aug. 1, 1992, p. L57-L59. Research supported by Unive

Astronomy and Astrophysics

Astrophysics

11

Stellar Winds, T Tauri Stars, Carbon Monoxide, Molecular Flow, Stellar Mass Ejection, Stellar Spectra

Scientific paper

Results are presented of 21-cm observations carried out in search of high-velocity H I gas in T Tauri. The results reveal the presence of an atomic gas of about 150-km/sec velocity, with an associated mass of 0.003 solar mass and a mass-loss rate of about 7 x 10 exp -7 solar mass/yr. It is suggested that the high-velocity neutral wind is the driving mechanism of the observed molecular outflow. The plausibility of this argument is supported by the report of Giovanardi et al. (1992), who detected a neutral atomic wind in L1551.

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