Observatory science with eXTP
Observatory science with eXTP
复制标题
使用 eXTP 进行观测科学
DOI：
10.1007/s11433-017-9186-1
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发表时间：
2019
期刊：
影响因子：
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通讯作者：
Rossi Elena
中科院分区：
文献类型：
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作者：
in't Z;Jean J M;Bozzo Enrico;Qu JinLu;Li Xiang Dong;Amati Lorenzo;Chen Yang;Donnarumma Immacolata;Doroshenko Victor;Drake Stephen A;Hernanz Margarita;Jenke Peter A;Maccarone Thomas J;Mahmoodifar Simin;de Martino Domitilla;De Rosa Aless;ra;Rossi Elena
在这份白色白皮书中，我们介绍了增强型X射线定时和偏振测量（eXTP）使命在与天文台科学目标相关的研究中的潜力。这些包括燃烧的恒星，超新星遗迹，吸积的白色矮星，低质量和高质量的X射线双星，射电安静和射电大声活动星系核，潮汐破裂事件和伽马射线爆发。eXTP将非常适合研究这些对象的一个共同方面：它们通常是瞬态的。由中国科学院高能物理研究所领导的国际联盟开发的eXTP使命预计将于2020年代中期发射。
In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Science, the eXTP mission is expected to be launched in the mid 2020s.