Effective temperatures of cool metal-poor stars derived from the analysis of 3D Balmer lines

AIP Conference Proceedings

Volumn 1094, Issue , 2009, Pages 784-787

  Behara, N T ^a   Ludwig, H G ^a   Steffen, M ^b   Bonifacio, P ^a,c  

^a OBSERVATOIRE DE PARIS   (France)

^b ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^c INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

Author keywords

Line: formation; Line: profiles; Stars: atmospheres; Stars: fundamental parameters

Indexed keywords

EID: 64849095157     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.3099233     Document Type: Conference Paper

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