On the structure of the accretion shock wave in the case of young stars

Details On the structure of the accretion shock wave in the case of young stars On the structure of the accretion shock wave in the case of young stars

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...295l..20l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 295, no. 2, p. L20-L22

Astronomy and Astrophysics

Astrophysics

35

Accretion Disks, Astronomical Models, Continuous Spectra, Emission Spectra, Shock Waves, Stellar Mass Accretion, T Tauri Stars, Magnetic Control, Mathematical Models, Optical Thickness, Stellar Magnetic Fields

Scientific paper

I argue that pre-shock zone is optically thin for continuum radiation
longward Lyman limit in the case of magnetically controlled disk
accretion onto low-mass young stars. The origin of the observed veiling
continuum and emission lines of classical T Tauri stars (CTTS) is
discussed.

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