Is there a hard tail in the Coma Cluster X-ray spectrum?
- Autor
- ROSSETTI, M1 2 ; MOLENDI, S1
[1] Istituto di Astrofisica Spaziale e Fisica Cosmica, via Bassini 15, 20133 Milano, Italy
[2] Università degli Studi di Milano, Dip. di Fisica, via Celoria 16, 20133 Milano, Italy - Fuente
Astronomy and astrophysics (Berlin. Print). 2004, Vol 414, Num 3, pp L41-L44 ; ref : 20 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- EDP Sciences, Les Ulis
- País de la publicación
- France
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave de autor
- X-rays: galaxies: clusters cosmic microwave background galaxies: clusters: individual: Coma magnetic field radiation mechanism: non-thermal
- Palabra clave (fr)
- Amas galaxies RX Champ magnétique Mécanisme rayonnement Rayonnement fond cosmique Rayonnement non thermique Spectre RX
- Palabra clave (in)
- X ray cluster of galaxies Magnetic fields Radiation mechanism Cosmic background radiation Nonthermal radiation X-ray spectra
- Palabra clave (es)
- Conglomerado galaxias RX Mecanismo radiación
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D65 Galaxy groups, clusters, and superclusters. Large-scale structure of the universe / 001E03D65C Galaxy clusters
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 15410347
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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DOI
10.1051/0004-6361:20031749 
https://dx.doi.org/10.1051/0004-6361:20031749
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