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1995A&A...295L..20L - Astronomy and Astrophysics, volume 295, L20-22 (1995/3-2)
On the structure of the accretion shock wave in the case of young stars.
LAMZIN S.A.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): accretion - shock waves - stars: pre-main-sequence
Simbad objects: 6
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