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
Abstract Accepted
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.  

 
Important Date
  • Conference Date

    May 12

    2025

    to

    May 15

    2025

  • Mar 26 2025

    Draft paper submission deadline

  • Apr 30 2025

    Early Bird Registration

  • May 15 2025

    Registration deadline

Sponsored By
Institute of Applied Physics and Computational Mathematics, Beijing, China
Shaanxi Normal University, Xi’an, China
Organized By
陕西师范大学
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