2508.17541
2026-06-03
astro-ph.HE
XRISM reveals a variable, multi-phase outflow-inflow structure during the X-ray obscured 2024 outburst of the black hole transient V4641 Sgr
XRISM揭示黑洞暂现源V4641 Sgr在2024年X射线掩蔽爆发期间的多相、变化的外流-内流结构
Maxime Parra, Megumi Shidatsu, Ryota Tomaru, Chris Done, Teo Muñoz-Darias, Montserrat Armas Padilla, Shoji Ogawa, Alessio Marino, Noa Grollimund, Stephane Corbel, Eduardo De la Fuente, Huaqing Cheng, María Díaz Trigo, Rob Fender, Keisuke Isogai, Shogo B. Kobayashi, Sara Motta, Katsuhiro Murata, Hitoshi Negoro, Samar Safi-Harb, Hiromasa Suzuki, Naomi Tsuji, Yoshihiro Ueda, Chen Zhang, Yuexin Zhang, Zuobin Zhang
AI总结
利用XRISM和Seimei望远镜对V4641 Sgr进行X射线和光学光谱观测,发现低光度爆发阶段存在高密度气体遮蔽内盘区域,并检测到复杂、不均匀的外流结构,包括显著红移和弱蓝移成分。