Non-LTE Balmer line formation in late-type spectra: Effects of atomic processes involving hydrogen atoms

Astronomy and Astrophysics

Volumn 466, Issue 1, 2007, Pages 327-337

  Barklem, P S ^a  

^a UPPSALA UNIVERSITY   (Sweden)

Author keywords

Line: formation

Indexed keywords

DATA ACQUISITION; ELECTRIC EXCITATION; HYDROGEN; RATE CONSTANTS; STARS; THERMODYNAMIC STABILITY;

BALMER LINE; EXPERIMENTAL DATA; LINE: FORMATION; SOLAR MODEL;

ATMOSPHERIC SPECTRA;

EID: 34250882128     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066686     Document Type: Article

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