094127
收藏DataCite Commons2026-03-09 更新2026-05-03 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/094127.html
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资源简介：
Several models recently proposed that QPEs are the electromagnetic counterpartof the GW emitters called extreme-mass ratio inspirals. We identified a way totest models proposing QPEs to be star-disk interactions by measuring the orbitaldecay driven by hydrodynamic drag induced on the star by the collisions with theaccretion disk surrounding the central black hole. We identify eRO-QPE2 as theideal candidate which allows a modest time request with XMM-Newton to make whatis perhaps the first major step forward in the newborn QPE field. We request 4observations for a total of 132ks. [truncated! Please see actual data for full text]
提供机构：
European Space Agency
创建时间：
2026-03-09
