Broadening of lines of Be II, Sr II and Ba II by collisions with hydrogen atoms and the solar abundance of strontium

Monthly Notices of the Royal Astronomical Society

Volumn 311, Issue 3, 2000, Pages 535-540

  Barklem, P S ^a   O'Mara, B J ^b  

^a BOX 515   (Sweden)

^b UNIVERSITY OF QUEENSLAND   (Australia)

Author keywords

Atomic data; Line: profiles; Sun: abundances

Indexed keywords

HYDROGEN; IONIZATION; SOLAR POWER GENERATION; STRONTIUM; STRONTIUM COMPOUNDS;

ABUNDANCE ANALYSIS; ATOMIC DATA; HYDROGEN ATOMS; IONIZED ATOM; LINE: PROFILES; NEUTRAL ATOMS; RESONANCE LINE; SOLAR ABUNDANCES; SPECTRAL LINE; SUN: ABUNDANCES;

ATOMS;

EID: 0007757246     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03090.x     Document Type: Article

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