会议专题

Optical Spectropolarimetry of Three microquasars, Cyg X-1, LS5039, LSI +61d303

We present optical spectropolarimetric observations of three microquasars, Cyg X-1, LS 5039 and LS I +61d 303. For Cyg X-1, the observed polarization shows time variation correlated with the orbital phase. For LS 5039, there is no evidence of intrinsic polarization. For LS I +61d 303, the result is consistent with that of 2005 Jan, Oct and Nov, except for the systematic decrease in the intrinsic polarization and in the EWs of the Ha emission line.

polarizatin binaries circumstellar matter scattering

O. Nagae K. S. Kawabata Y. Fukazawa A. Okazaki M. Isogai

Hiroshima University, Higaski-hiroshima, Hiroshima, Japan Hiroshima Astrophysical Science Center, Hiroshima University Hiroshima University Gunma University, Maebashi Gunma, Japan

国际会议

紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)

安徽黄山

英文

328-330

2007-07-01(万方平台首次上网日期,不代表论文的发表时间)