메뉴 건너뛰기




Volumn 396, Issue 3, 2009, Pages 1743-1763

3D models of radiatively driven colliding winds in massive O+O star binaries - I. Hydrodynamics

Author keywords

Binaries: general; Hydrodynamics; Shock waves; Stars: early type; Stars: mass loss; Stars: winds, outflows

Indexed keywords

COLLISIONAL PLASMAS; COOLING; HYDRODYNAMICS; SHOCK WAVES; SPEED; STARS;

EID: 67549144061     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14857.x     Document Type: Article
Times cited : (128)

References (68)
  • 16
    • 11944272488 scopus 로고
    • Gayley K. G., 1995, ApJ, 454, 410
    • (1995) ApJ , vol.454 , pp. 410
    • Gayley, K.G.1
  • 30
    • 0031509942 scopus 로고    scopus 로고
    • Lührs S., 1997, PASP, 109, 504
    • (1997) PASP , vol.109 , pp. 504
    • Lührs, S.1
  • 33
    • 12044250002 scopus 로고
    • Masai K., 1994, ApJ, 437, 770
    • (1994) ApJ , vol.437 , pp. 770
    • Masai, K.1
  • 35
    • 18044402260 scopus 로고    scopus 로고
    • Morrell N. I. et al., 2001, MNRAS, 326, 85
    • (2001) MNRAS , vol.326 , pp. 85
    • Morrell, N.I.1
  • 40
  • 41
    • 0009752687 scopus 로고    scopus 로고
    • in. van der Hucht, K. A. Koenigsberger, G. Eenens, P. R. J. eds, IAU Symp. No. 193. Astron. Soc. Pac. San Francisco. p.
    • Pittard J. M., 1999, in van der Hucht K. A., Koenigsberger G., Eenens P. R. J., eds, IAU Symp. No. 193, Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies. Astron. Soc. Pac., San Francisco, p. 386
    • (1999) Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies. , pp. 386
    • Pittard, J.M.1
  • 42
    • 34249867171 scopus 로고    scopus 로고
    • Pittard J. M., 2007, ApJ, 660, L141
    • (2007) ApJ , vol.660 , pp. 141
    • Pittard, J.M.1
  • 65
    • 12044254002 scopus 로고
    • Vishniac E. T., 1994, ApJ, 428, 186
    • (1994) ApJ , vol.428 , pp. 186
    • Vishniac, E.T.1
  • 66
    • 0002622922 scopus 로고    scopus 로고
    • Walder R., 1998, Ap&SS, 260, 243
    • (1998) Ap&SS , vol.260 , pp. 243
    • Walder, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.