Renewed Activity from the X-Ray Transient SAXJ 1810.8-2609 with Integral

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Auteur(s):

Editeur:

HAL CCSD

American Astronomical Society

Contributeur:

Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma) ; INAF

Technical University of Denmark [Lyngby ] ; Technical University of Denmark

INAF-IASF/Rome ; INAF

AstroParticule et Cosmologie (APC - UMR 7164) ; CNRS - CEA - IN2P3 - Observatoire de Paris - Université Paris Diderot - Paris 7 (UP7)

Université de Genève (UNIGE)

Astronomical Institute, Academy of Sciences ; Astronomical Institute, Academy of Sciences

Langue:

ANGLAIS

Candidats descripteurs:

gamma rays: observations

radiation mechanisms: non-thermal

stars: individual: SAX J1810.8-2609

stars: neutron

X-rays: binaries

[PHYS.ASTR.HE] Physics/Astrophysics/High Energy Astrophysical Phenomena

[SDU.ASTR.HE] Sciences of the Universe/Astrophysics/High Energy Astrophysical Phenomena

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