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Volumn 539, Issue , 2012, Pages

3D simulations of microquasar jets in clumpy stellar winds

Author keywords

hydrodynamics; ISM: jets and outflows; radiation mechanisms: general; shock waves; stars: winds, outflows; X rays: binaries

Indexed keywords

3D SIMULATIONS; COMPACT OBJECTS; FILLING FACTOR; HIGHER-DEGREE; INHOMOGENEITIES; ISM: JETS AND OUTFLOWS; JET VELOCITIES; MASSIVE STARS; MICROQUASARS; RADIATION MECHANISMS: GENERAL; RADIO JET; SOUND SPEED; STARS: WINDS, OUTFLOWS; STELLAR WIND; THREE-DIMENSIONAL NUMERICAL SIMULATIONS; X-RAYS: BINARIES;

EID: 84857437044     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118262     Document Type: Article
Times cited : (47)

References (33)
  • 5
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    • Barkov, M. V., & Khangulyan, D. 2012, MNRAS, in press [arXiv:astro-ph/1109.5810]
    • (2012) MNRAS
    • Barkov, M.V.1    Khangulyan, D.2
  • 28
    • 33750029415 scopus 로고    scopus 로고
    • Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA
    • Ribó, M. 2005, in Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conf. Proc., 340, 269
    • (2005) ASP Conf. Proc. , vol.340 , pp. 269
    • Ribó, M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.