Stochastic models of stellar winds in T Tauri-stars

Details Stochastic models of stellar winds in T Tauri-stars Stochastic models of stellar winds in T Tauri-stars

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185..107g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 1, Nov. 1991, p. 107-127. Translation.

Astronomy and Astrophysics

Astrophysics

19

Astronomical Models, Emission Spectra, Stellar Winds, Stochastic Processes, T Tauri Stars, H Alpha Line, Line Spectra, Magnesium, Metallicity

Scientific paper

The conditions in which emission lines of hydrogen, ionized calcium, and ionized magnesium are formed in the spectra of T-Tauri stars are considered. It is found that the structural characteristics of winds from T Tauri stars are very different from those which are represented in models of an expanding continuous medium. Mass loss from a T Tauri star is an extremely nonuniform process over the surface, apparently embodying a real inhomogeneity in magnetic activity on the stellar surface.

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