The importance of a correct abundance assumption in determining the effective temperature and gravity of stars: A spectroscopic study of the helium weak stars HD 5737, HD 175362 and HD 202671

Astronomy and Astrophysics

Volumn 320, Issue 1, 1997, Pages 257-264

  Leone, F ^a   Manfre M ^b  

^a Citta' Universitaria   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

Line: identification; Stars: abundances; Stars: chemically peculiar; Stars: individual: HD 5737, HD 175362 and HD 202671

Indexed keywords

EID: 0009702916     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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