Formation of Fe X-Fe XIV coronal lines in the accretion shock of T Tauri stars

Astronomy and Astrophysics

Volumn 369, Issue 3, 2001, Pages 965-970

  Lamzin, S A ^a   Stempels, H C ^b   Piskunov, N E ^b  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

^b BOX 515   (Sweden)

Author keywords

Physical processes: accretion discs; Physical processes: line formation; Physical processes: shock waves; Stars: individual: RU Lup, RY Tau, DF Tau; Stars: pre main sequence

Indexed keywords

EID: 0035298302     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010159     Document Type: Article

References (18)