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26–28 Apr 2008
中国科学院上海天文台
Asia/Shanghai timezone
Local Organization Committee

Simulations on millimeter and sub-millimeter emission from Sagittarius A*

Not scheduled
三楼报告厅 (中国科学院上海天文台)

三楼报告厅

中国科学院上海天文台

上海市徐汇区南丹路80号 邮编:200030

Speaker

Ms Lei Huang (PhD. Student)

Summary

Our best-fit model can reproduce the spectrum and polarization of Sgr A* in
millimeter and shorter wavlengths and further predicts distinct LP and CP at ~1THz.
The model constraints the inclination angle of the MRI-driven torus as $40^\circ \pm 10^\circ$, and the position angle $120^\circ \pm 30^\circ$.

Primary author

Ms Lei Huang (PhD. Student)

Presentation materials

There are no materials yet.