086191
收藏DataCite Commons2023-04-21 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/086191.html
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资源简介：
A new type of X-ray transients was very recently discovered and named X-ray Quasi-Periodic Eruptions openParQPEsclosePar. This phenomenon likely traced comma around a black hole openParBHclosePar of a few hundred thousands solar masses comma the ongoing formation and stabilization of an accretion flow analogous to the one that we observed in more massive sources. Combining the scanning capabilities of eROSITA comma launchen in July 2019 comma with subsequent deeper XMM-Newton observations comma we can continuously identify QPE candidates with the former and confirm their nature with the latter. This synergy will provide precious insights on BH growth and evolution.
提供机构：
European Space Agency
创建时间：
2023-04-21
