A study of π Aquarii during a quasi-normal star phase: Refined fundamental parameters and evidence for binarity

Astrophysical Journal

Volumn 573, Issue 2 I, 2002, Pages 812-824

  Bjorkman, Karen S ^a   Miroshnichenko, Anatoly S ^a   McDavid, David ^b   Pogrosheva, Tatiana M ^c  

^a UNIVERSITY OF TOLEDO   (United States)

^b Limber Observatory   (United States)

^c MOSCOW STATE UNIVERSITY   (Russian Federation)

Author keywords

Binaries: spectroscopic; Circumstellar matter; Stars: emission line, Be; Stars: individual ( Aquarii); Techniques: photometric; Techniques: spectroscopic

Indexed keywords

EID: 0042528197     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/340751     Document Type: Article

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