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Comparison of approximately isothermal gravitational potentials of elliptical galaxies based on X-ray and optical data

Author
CHURAZOV, E1 2 ; TREMAINE, S3 ; FORMAN, W4 ; GERHARD, O5 ; DAS, P5 ; VIKHLININ, A2 4 ; JONES, C4 ; BÖHRINGER, H5 ; GEBHARDT, K6
[1] Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
[2] Space Research Institute (IKI), Profsoyuznaya 84/32, Moscow 117810, Russian Federation
[3] Institute for Advanced Study, Einstein Dr., Princeton, NJ 08540, United States
[4] Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, United States
[5] MPI für Extraterrestrische Physik, PO Box 1603, 85740 Garching, Germany
[6] Department of Astronomy, University of Texas, Austin, TX 78712, United States
Source

Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 404, Num 3, pp 1165-1185, 21 p ; ref : 3/4 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Wiley-Blackwell, Malden, MA
Publication country
United States
Document type
Article
Language
Russian
Author keyword
X-rays: galaxies: clusters galaxies: kinematics and dynamics
Keyword (fr)
Amas galaxies RX Brillance surface Cinématique Dispersion vitesse Dynamique Estimateur Galaxies elliptiques Gaz chaud Incertitude Observation RX Observation optique Potentiel gravitationnel Source RX cosmique Sphère
Keyword (en)
X ray cluster of galaxies Surface brightness Kinematics Velocity dispersion Dynamics Estimator Elliptical galaxies Hot gas Uncertainty X ray observation Optical observation Gravitational potential Cosmic x-ray sources Spheres
Keyword (es)
Conglomerado galaxias RX Brillantez superficie Dispersión velocidad Estimador Gas caliente Incertidumbre Observación RX Observación óptica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22774723

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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