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Volumn 418, Issue 1, 2004, Pages 151-162

Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?

Author keywords

Infrared: stars; Radiative transfer; Stars: circumstellar matter; Stars: individual: Orionis, SW Virginis, R Leonis; Stars: late type; Techniques: interferometric

Indexed keywords

ASYMPTOTIC STABILITY; CONDENSATION; DUST; INFRARED RADIATION; INTEGRAL EQUATIONS; INTERFEROMETERS; INTERFEROMETRY; MATHEMATICAL MODELS; PHOTOMETRY; TURBULENCE; VISIBILITY;

EID: 2142836544     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040057     Document Type: Article
Times cited : (16)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.