X-ray flares in Orion young stars. I.

B2FIND2026-03-19 收录

恒星X射线观测

年轻恒星活动

数据链接：

https://b2find.eudat.eu/dataset/887da486-adda-5a50-8236-67a190f05516 数据链接链接失效反馈

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Pre-main-sequence (PMS) stars are known to produce powerful X-ray flares, which resemble magnetic reconnection solar flares scaled by factors up to 104. However, there are...

主序前星（Pre-main-sequence (PMS) stars）已知会产生强烈的X射线耀斑，此类耀斑与经最高达10⁴倍缩放的磁重联太阳耀斑高度相似。然而目前仍存在……

X-ray flares in Orion young stars. I.

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