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MODELS OF TYPE I X-RAY BURSTS FROM GS 1826-24 : A PROBE OF rp-PROCESS HYDROGEN BURNING

Author
HEGER, Alexander1 ; CUMMING, Andrew2 ; GALLOWAY, Duncan K3 ; WOOSLEY, Stanford E4
[1] Theoretical Astrophysics Group, T-6, MS B227, Los Alamos National Laboratory, Los Alamos, NM 87545, United States
[2] Department of Physics, McGill University, Montreal QC, H3A 2T8, Canada
[3] School of Physics, University of Melbourne, Victoria, Australia
[4] Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, United States
Source

The Astrophysical journal. 2007, Vol 671, Num 2 ; L141-L144 ; 2 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
accretion, accretion disks stars: individual (Ginga 1826-238, GS 1826-24) stars: neutron-X-rays: bursts
Keyword (fr)
Combustion hydrogène Disque accrétion Etoile neutron Modèle Source RX cosmique Sursaut RX type I Sursaut RX
Keyword (en)
Hydrogen burning Accretion disks Neutron stars Models Cosmic x-ray sources Type I X ray burst X ray burst
Keyword (es)
Modelo Arrebato RX tipo I Arrebato RX
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19954673

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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