메뉴 건너뛰기




Volumn 388, Issue 3, 2002, Pages 957-977

Mass-loss rate determination for the massive binary V444 Cygni using 3-D Monte-Carlo simulations of line and polarization variability

Author keywords

Polarization; Stars: binaries: eclipsing; Stars: individual: V444 Cygni; Stars: mass loss; Stars: Wolf Rayet

Indexed keywords

COMPUTER SIMULATION; CURVE FITTING; GALAXIES; MATHEMATICAL MODELS; MONTE CARLO METHODS; POLARIZATION;

EID: 0036611886     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020443     Document Type: Article
Times cited : (24)

References (72)
  • 46
    • 0040415082 scopus 로고    scopus 로고
    • Polarized radiation of circumstellar origin
    • ed. G.V. Coyne, A.M. Magalhães A. F. J. Moffat, et al. (Vatican City State: Vatican Observatory)
    • Piirola, V.1    Linnaluoto, S.2
  • 50
    • 0009752687 scopus 로고    scopus 로고
    • Wolf-Rayet phenomena in massive stars and starburst galaxies
    • ed. K. A. van der Hucht, G. Koenigsberger, & P.R.J. Eenens (San Francisco: Astronomical Society of the Pacific)
    • (1999) IAU Symp. , vol.193 , pp. 386
    • Pittard, J.M.1    Stevens, I.R.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.