High-resolution spectroscopy of Vega-like stars - I. Effective temperatures, gravities and photospheric abundances

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 3, 1997, Pages 604-616

  Dunkin, S K ^a   Barlow, M J ^a   Ryan, Sean G ^b  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b ANGLO AUSTRALIAN OBSERVATORY   (Australia)

Author keywords

Stars: abundances; Stars: fundamental parameters; Stars: pre main sequence

Indexed keywords

DUST; ELECTROMAGNETIC WAVE EMISSION; INFRARED RADIATION; SPECTROSCOPIC ANALYSIS; TEMPERATURE; THERMAL LOGGING;

CIRCUMSTELLAR; DUST EMISSION; EFFECTIVE TEMPERATURE; MAIN SEQUENCE STARS; PROPERTY; SPECTRAL TYPES; STARS ABUNDANCES; STARS: BE; STARS: PRE-MAIN SEQUENCE; STARS:FUNDAMENTAL PARAMETERS;

STARS;

EID: 0001068831     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.3.604     Document Type: Article

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