SCOPUS 정보 검색 플랫폼

Astronomy and Astrophysics

Volumn 389, Issue 1, 2002, Pages 162-179

The mass-loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models

(2) Nugis, T a Lamers, H J G L M b,c

a TARTU OBSERVATORY (Estonia)

b UTRECHT UNIVERSITY (Netherlands)

c SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH (Netherlands)

Author keywords

Stars: atmospheres; Stars: emission lines; Stars: evolution; Stars: mass loss; Stars: Wolf Rayet

Indexed keywords

GALAXIES; MASS TRANSFER; OPACITY; WIND EFFECTS;

STARS;

ASTROPHYSICS;

EID: 0036304117 PISSN: 00046361 EISSN: None Source Type: Journal
DOI: 10.1051/0004-6361:20020557 Document Type: Article

Times cited : (111)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.