Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7156
Title: Observatory science with eXTP
Authors: Enrico, Bozzo
JinLu, Qu
Paul, Biswajit
+ 152 Co-Authors
Keywords: space research instruments
nuclear astrophysics
flare stars
accretion and accretion disks
mass loss and stellar winds
X-ray binaries
Issue Date: Feb-2019
Publisher: Science China Press
Citation: Science China Physics, Mechanics & Astronomy, Volume 62, AR 29506, 42 pp.
Abstract: 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. EXP 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.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/7156
ISSN: 1674-7348
1869-1927(Online)
Alternative Location: https://ui.adsabs.harvard.edu//#abs/2019SCPMA..6229506I/abstract
https://arxiv.org/abs/1812.04023
https://doi.org/10.1007/s11433-017-9186-1
Copyright: © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2019
Appears in Collections:Research Papers (A&A)

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