On the shock-induced variability of emission lines in M-type mira variables II. Fe II and [Fe II] emission lines as a diagnostic tool

Astronomy and Astrophysics

Volumn 400, Issue 1, 2003, Pages 319-328

  Richter, He ^a   Wood, P R ^b   Woitke, P ^a   Bolick, U ^a   Sedlmayr, E ^a  

^a TECHNISCHE UNIVERSITÄT BERLIN   (Germany)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Line: Formation; Radiative transfer; Shock waves; Stars: Late type; Stars: Variables: General

Indexed keywords

CALCULATIONS; GALAXIES; HYDRODYNAMICS; IONIZATION; LIGHT EMISSION; MATHEMATICAL MODELS; SHOCK WAVES; THERMODYNAMICS;

NONLOCAL THERMODYNAMIC EQUILIBRIUM; PHOTOSPHERE; RADIATIVE TRANSFER;

ASTROPHYSICS;

EID: 0037337735     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021862     Document Type: Article

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