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Observatory science with eXTP
DOI:10.1007/s11433-017-9186-1.png)
摘要
En 中文
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.
Keyword:
space research instruments
nuclear astrophysics
flare stars
accretion and accretion disks
mass loss and stellar winds
cataclysmic binaries
X-ray binaries
supernova remnants
active galactic nuclei
X-ray bursts
gamma-ray bursts
gravitational waves
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被引数:
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引用论文
Short-period X-ray oscillations in super-soft novae and persistent super-soft sources超软新星和持久超软源中的短周期x射线振荡

