The angular sizes of dwarf stars and subgiants: Non-linear surface brightness relations in BVRcIc from interferometry

Astronomy and Astrophysics

Volumn 491, Issue 3, 2008, Pages 855-858

  Kervella, P ^a   Fouque P ^b  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITÉ DE TOULOUSE   (France)

Author keywords

Stars: fundamental parameters; Techniques: interferometric

Indexed keywords

COLOR; FORECASTING; INTERFEROMETERS; INTERFEROMETRY; MARINE MISSILES; OPTICAL PROPERTIES; PHOTOMETERS; PHOTOMETRY; POLYNOMIAL APPROXIMATION; POLYNOMIALS; TELECOMMUNICATION SYSTEMS;

ACCURATE PREDICTIONS; ANGULAR DIAMETERS; ANGULAR SIZES; APPLICATIONS.; BASE-LINES; BASELINE INTERFEROMETRIES; DWARF STARS; EFFECTIVE TEMPERATURES; EXTRASOLAR PLANETS; LINEAR SURFACES; POLYNOMIAL FITS; POLYNOMIAL RELATIONS; SPECTRAL FEATURES; STARS: FUNDAMENTAL PARAMETERS; SUBGIANTS; SURFACE BRIGHTNESSES; TECHNIQUES: INTERFEROMETRIC;

STARS;

EID: 57049091791     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810317     Document Type: Article

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