Detecting faint secondaries of spectroscopic binaries: HD 101177B and 149414A

Monthly Notices of the Royal Astronomical Society

Volumn 284, Issue 2, 1997, Pages 341-347

  Mazeh, T ^a,b   Martin E L ^c   Goldberg, D ^a   Smith, H A ^b  

^a TEL AVIV UNIVERSITY   (Israel)

^b SMITHSONIAN INSTITUTION   (United States)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

Author keywords

Binaries: spectroscopic; Stars: individual: HD 101177B; Stars: individual: HD 149414A

Indexed keywords

STARS;

BINARIES: SPECTROSCOPIC; HIGH SIGNAL-TO-NOISE RATIO; MASS RATIO; RADIAL VELOCITY; RATIO SPECTRA; SPECTROSCOPIC BINARY; STAR: INDIVIDUAL: HD 101177B; STAR: INDIVIDUAL: HD 149414A; STARS: INDIVIDUAL: PROXIMA CENTAURI;

SIGNAL TO NOISE RATIO;

EID: 0012447574     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/284.2.341     Document Type: Article

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