178 / 2025-03-18 10:34:01
Laboratory study the X-ray emission of knots in Young Stellar Objects
X-ray emission;,YSO jet,high power laser
摘要录用
魏会冈 / 中国科学院国家天文台
Jets are excellent probes to study the evolution of protostars since they carry along the fossil information on the beginning of star formation. Recent observations have shown that X-ray emission and high energy particles exist in Young Stellar Objects (YSOs) jets and their knots. However, the mechanisms for plasma heating and particle acceleration are not clearly verified. In this presentation, we will introduce our recent experimental results on the reproduction of knots in YSO jets with intense lasers in laboratory. X-ray emission and electron energy spectra are both obtained. We have also proposed a new model to explain the shock formation and the heating of the plasma.  

 
重要日期
  • 会议日期

    05月12日

    2025

    05月15日

    2025

  • 03月26日 2025

    初稿截稿日期

  • 04月30日 2025

    提前注册日期

  • 05月15日 2025

    注册截止日期

主办单位
北京应用物理与计算数学研究所
陕西师范大学
承办单位
陕西师范大学
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