Observatory science with eXTP

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In't Zand, Jean J. M. and Kalemci, Emrah (2019) Observatory science with eXTP. Science China: Physics, Mechanics & Astronomy (SI), 62 (2). ISSN 1674-7348 (Print) 1869-1927 (Online)

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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. 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.
Item Type: Article
Additional Information: Group of authors / WoS & Scopus Document Type: Review
Uncontrolled Keywords: 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
Subjects: Q Science > QB Astronomy > QB460-466 Astrophysics
Divisions: Faculty of Engineering and Natural Sciences > Basic Sciences > Physics
Faculty of Engineering and Natural Sciences
Depositing User: Emrah Kalemci
Date Deposited: 23 Aug 2019 12:14
Last Modified: 26 Apr 2022 10:06
URI: https://research.sabanciuniv.edu/id/eprint/37603

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