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Entropy floor and effervescent heating of intracluster gas

Author
ROYCHOWDHURY, S; RUSZKOWSKI, M1 ; NATH, B. B; BEGELMAN, Mitchell C1 2
Raman Research Institute, Sadashivanagar, Bangalore 560080, India
[1] JILA, Campus Box 440, University of Colorado at Boulder, CO 80309-0440, United States
[2] Department of Astrophysical and Planetary Sciences, University of Colorado at Boulder, United States
Source

The Astrophysical journal. 2004, Vol 615, Num 2, pp 681-688, 8 p ; 1 ; ref : 55 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)
Amas galaxies RX Entropie Gaz intergalactique Matière intergalactique Matière intraamas Ecoulement refroidissement
Keyword (en)
X ray cluster of galaxies Entropy Intergalactic gas Intergalactic matter Intracluster matter Cooling flow
Keyword (es)
Conglomerado galaxias RX Gas intergaláctico Materia intracúmulo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A30 Fundamental aspects of astrophysics / 001E03A30T Thermodynamic processes, conduction, convection, equations of state

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 / 001E03D65H Intracluster matter ; cooling flows

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16358960

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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