The case for anisotropic mass loss from T Tauri stars

Details The case for anisotropic mass loss from T Tauri stars The case for anisotropic mass loss from T Tauri stars

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..266c&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Apr. 1982, p. 266-270.

Astronomy and Astrophysics

Astronomy

35

Anisotropic Media, Stellar Mass Ejection, T Tauri Stars, Carbon Monoxide, Cosmic Dust, Herbig-Haro Objects, Mass Flow Rate, Radio Emission, Stellar Structure

Scientific paper

Observational evidence and theoretical arguments are assembled in favor of directed, rather than isotropic, mass flows from T Tauri stars. These arguments include the structure of T Tauri nebulosities, radio continuum maps of the stars, the motions of Herbig-Haro objects away from their exciting T Tauri stars, bipolar CO flows, and particularly the spatial coincidence of an optical jet and radio emission associated with an embedded, probably T Tauri star in the dark cloud L1551.

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