RX j1821.6+6827: A cool cluster at z = 0.81 from the ROSAT NEP survey
- Author
- GIOIA, I. M1 ; WOLTER, A2 ; MULLIS, C. R3 ; HENRY, J. P4 ; BÖHRINGER, H5 ; BRIEL, U. G5
[1] Istituto di Radioastronomia CNR, via P. Gobetti 101, 40129 Bologna, Italy
[2] INAF, Osservatorio Astronomico di Brera, via Brera 28, 20121 Milano, Italy
[3] European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching bei, München 85740, Germany
[4] Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, United States
[5] Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse, Postfach 1312, Garching 85741, Germany - Source
Astronomy and astrophysics (Berlin. Print). 2004, Vol 428, Num 3, pp 867-875, 9 p ; ref : 60 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- X-rays: galaxies: clusters X-rays: general X-rays: individuals: RX J1821.6+6827 galaxies: clusters: general galaxies: clusters: individual: RX J1821.6+6827 galaxies: intergalactic medium
- Keyword (fr)
- Abondance Amas galaxies RX Amas galaxies Amas local Cosmologie Dispersion vitesse Déplacement vers le rouge Emission RX Etude ciel Galaxies Incertitude Loi puissance Luminosité Matière intergalactique Modèle Noyau galactique actif Source ponctuelle
- Keyword (en)
- Abundance X ray cluster of galaxies Galaxy clusters Local cluster Cosmology Velocity dispersion Red shift X ray emission Sky surveys Galaxies Uncertainty Power law Luminosity Intergalactic matter Models Active galaxy nuclei Point sources
- Keyword (es)
- Conglomerado galaxias RX Cúmulo local Dispersión velocidad Emisión RX Incertidumbre Ley poder Modelo
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16331998
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
10.1051/0004-6361:20041426 
https://dx.doi.org/10.1051/0004-6361:20041426
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