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High-energy gamma rays from stellar associations

Author
TORRES, Diego F1 ; DOMINGO-SANTAMARIA, Eva2 ; ROMERO, Gustavo E3
[1] Lawrence Livermore National Laboratory, 7000 East Avenue, L-413, Livermore, CA 94550, United States
[2] Institut de Física d'Altes Energies (IFAE), Edifici C-n, Campus UAB, 08193 Bellaterra, Spain
[3] Instituto Argentino de Radioastronomía (IAR), C.C. 5, 1894, Villa Elisa, Argentina
Source

The Astrophysical journal. 2004, Vol 601, Num 1, pp L75-L78 ; 2 ; ref : 39 ref

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
Keyword (fr)
Association stellaire OB Domaine énergie TeV Etoile premier type Neutrino cosmique Rayonnement cosmique Rayonnement gamma Source Rγ galactique Vent stellaire
Keyword (en)
OB stellar association TeV range Early type stars Cosmic neutrinos Cosmic radiation Gamma radiation Galactic γ ray source Stellar winds
Keyword (es)
Asociación estelar OB Fuente Rγ galáctica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D20 Stellar clusters and associations / 001E03D20A Associations of stars (ob, t, r) in the milky way

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D70 Unidentified sources and radiation outside the solar system / 001E03D70R Gamma-ray sources ; gamma-ray bursts

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
15997682

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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