Theoretical oscillator strengths for Sr II and Y III, with application to abundances in the HgMn-type star χ Lupi

Astrophysical Journal

Volumn 496, Issue 2 PART I, 1998, Pages 1051-1057

  Brace, Tomas ^a,b   Wahlgren, Glenn M ^a,b   Johansson, Sveneric G ^b,c   Leckrone, David S ^d   Proffitt, Charles R ^a  

^a Computer Sciences Corporation ^*  (United States)

^b LUND UNIVERSITY   (Sweden)

^c LUND UNIVERSITY   (Sweden)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Aomic data; Stars: abundances; Stars: individual ( Lupi)

Indexed keywords

EID: 0001711824     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/305401     Document Type: Article

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