磁場方向在絲狀雲中恆星形成率的影響


物理系學生會議:磁場方向在絲狀雲中恆星形成率的影響

Talk:- The Effect of Magnetic Field Orientation on Star Formation Rate in Filament Clouds

With the rapid growth of computational power, numerical simulation has become more and more important in astrophysical researches in the last few decades. In this presentation, we will briefly introduce the simulation we are adopting in our group, as well as one of the currently undergoing simulation projects, aiming to reveal the effect of magnetic field orientation and other effects on star formation rate in filament clouds. The importance of magnetic field orientation in star formation has been gradually realised in the recent decades. However, the effect of different orientations on star formation rate in particular types of filaments is still yet to be understood, which will be the central topic of the project. 
 
時間:2017.05.20(六) 15:45 ~ 16:00
地點:香港中文大學 科學館LT4
講者:GUO Zitan
語言:英語

#131

此活動由香港中文大學物理系主辦。

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