The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii

Astronomy and Astrophysics

Volumn 554, Issue , 2013, Pages

  Arroyo Torres, B ^a   Wittkowski, M ^b   Marcaide, J M ^a   Hauschildt, P H ^c  

^a UNIVERSITY OF VALENCIA   (Spain)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Hertzsprung Russell and C M diagrams; Stars: atmospheres; Stars: fundamental parameters; Stars: individual: AH Scorpii; Stars: individual: KW Sagittarii; Stars: individual: UY Scuti

Indexed keywords

EFFECTIVE TEMPERATURE; FUNDAMENTAL PROPERTIES; HERTZSPRUNG-RUSSELL AND C-M DIAGRAMS; HYDROSTATIC ATMOSPHERIC MODEL; NEAR INFRARED SPECTRA; STARS: ATMOSPHERE; STARS: INDIVIDUAL; STARS:FUNDAMENTAL PARAMETERS;

ATMOSPHERIC STRUCTURE; HYDRAULICS; HYDRODYNAMICS; INFRARED DEVICES; STARS;

VISIBILITY;

EID: 84878846625     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220920     Document Type: Article

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