Observatory science with eXTP

Angelo Francesco Gambino, Rosario Iaria, Tiziana Di Salvo

Risultato della ricerca: Book/Film/Article review

11 Citazioni (Scopus)

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.
Lingua originaleEnglish
Numero di pagine42
RivistaDefault journal
Volume62
Stato di pubblicazionePublished - 2019

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cita questo

Observatory science with eXTP. / Gambino, Angelo Francesco; Iaria, Rosario; Di Salvo, Tiziana.

In: Default journal, Vol. 62, 2019.

Risultato della ricerca: Book/Film/Article review

Gambino, AF, Iaria, R & Di Salvo, T 2019, 'Observatory science with eXTP', Default journal, vol. 62.
Gambino AF, Iaria R, Di Salvo T. Observatory science with eXTP. Default journal. 2019;62.
Gambino, Angelo Francesco ; Iaria, Rosario ; Di Salvo, Tiziana. / Observatory science with eXTP. In: Default journal. 2019 ; Vol. 62.
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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.",
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AU - Gambino, Angelo Francesco

AU - Iaria, Rosario

AU - Di Salvo, Tiziana

PY - 2019

Y1 - 2019

N2 - 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.

AB - 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.

KW - Physics and Astronomy (all)

KW - X-ray binaries

KW - X-ray bursts

KW - accretion and accretion disks

KW - active galactic nuclei

KW - cataclysmic binaries

KW - flare stars

KW - gamma-ray bursts

KW - gravitational waves

KW - mass loss and stellar winds

KW - nuclear astrophysics

KW - space research instruments

KW - supernova remnants

UR - http://hdl.handle.net/10447/338145

UR - http://www.springer.com/physics/journal/11433

M3 - Book/Film/Article review

VL - 62

JO - Default journal

JF - Default journal

ER -

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