The ability of intermediate-band Strömgren photometry to correctly identify dwarf, subgiant, and giant stars and provide stellar metallicities and surface gravities

Astronomy and Astrophysics

Volumn 521, Issue 5, 2010, Pages

  Arnadottir A S ^a   Feltzing, S ^a   Lundstrom I ^a  

^a LUND UNIVERSITY   (Sweden)

Author keywords

Galaxy: stellar content; Solar neighborhood; Stars: abundances; Stars: fundamental parameters

Indexed keywords

BROAD BANDS; DWARF STARS; GALAXY:STELLAR CONTENT; GENERALISATION; GIANT STARS; HIGH RESOLUTION; HIGH SIGNAL-TO-NOISE RATIO; INTERMEDIATE BANDS; METALLICITIES; MILKY WAYS; SOLAR NEIGHBORHOOD; SPECTROSCOPIC SURVEYS; STARS: ABUNDANCES; STARS: FUNDAMENTAL PARAMETERS; STELLAR PARAMETERS; SURFACE GRAVITY;

CALIBRATION; FADING (RADIO); GALAXIES; LIBRARIES; PHOTOMETERS; PHOTOMETRY; SIGNAL TO NOISE RATIO; STANDARDS; SURVEYS;

STARS;

EID: 77958145101     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913544     Document Type: Article

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