Is Arcturus a well-understood K giant? Test of model atmospheres and potential companion detection by near-infrared interferometry

Astronomy and Astrophysics

Volumn 435, Issue 1, 2005, Pages 289-301

  Verhoelst, T ^a,c   Borde P J ^b   Perrin, G ^c   Decin, L ^a   Eriksson, K ^d   Ridgway, S T ^c,e   Schuller, P A ^b   Traub, W A ^b   Millan Gabet, R ^e   Lacasse, M G ^b   Waelkens, C ^a  

^a KU LEUVEN   (Belgium)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d Box 515   (Sweden)

^e NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

Author keywords

Stars: atmospheres; Stars: binaries: general; Stars: individual: Arcturus; Techniques: interferometric

Indexed keywords

APPROXIMATION THEORY; ASTROPHYSICS; CALIBRATION; DATA REDUCTION; INFRARED SPECTROPHOTOMETERS; MATHEMATICAL MODELS; PHOTOMETRY; THERMODYNAMICS;

STARS: ATMOSPHERES; STARS: BINARIES: GENERAL; STARS: INDIVIDUAL: ARCTURUS; TEACHNIQUES: INTERFEROMETRIC;

INTERFEROMETRY;

EID: 20844452217     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042356     Document Type: Article

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