The neon content of nearby B-type stars and its implications for the solar model problem

Astronomy and Astrophysics

Volumn 487, Issue 1, 2008, Pages 307-315

  Morel, T ^a,b   Butler, K ^c  

^a UNIVERSITY OF LIÈGE   (Belgium)

^b KU LEUVEN   (Belgium)

^c UNIVERSITY OF MUNICH   (Germany)

Author keywords

Stars: abundances; Stars: atmospheres; Stars: early type; Stars: fundamental parameters; Sun: helioseismology

Indexed keywords

INERT GASES; STARS; WELL TESTING;

CHEMICAL EVOLUTION; DIRECT ANALYSIS; HELIOSEISMOLOGY; INTERNAL STRUCTURES; INTERSTELLAR GASES; LOCAL INTERSTELLAR MEDIUM; OPTICAL (PET) (OPET); SOLAR ABUNDANCES; SOLAR MODEL PROBLEM; SOLAR MODELING; SOLAR NEIGHBOURHOOD; STELLAR OBJECTS;

NEON;

EID: 48249148779     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809924     Document Type: Article

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