Method for calculating the opacity of the atomic lines in stellar atmospheres

Astrophysical Journal

Volumn 690, Issue 2, 2009, Pages 1378-1385

  Cardona, O ^a   Simonneau, E ^b   Crivellari, L ^c  

^a INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^b CNRS   (France)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

Author keywords

Atomic processes; Line: formation; Stars: atmospheres

Indexed keywords

EID: 62549148681     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/690/2/1378     Document Type: Article

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