CONSTRAINTS ON THE SELF-INTERACTION CROSS SECTION OF DARK MATTER FROM NUMERICAL SIMULATIONS OF THE MERGING GALAXY CLUSTER 1E 0657-56
- Author
- RANDALL, Scott W1 ; MARKEVITCH, Maxim1 2 ; CLOWE, Douglas3 4 ; GONZALEZ, Anthony H5 ; BRADAC, Marusa6
[1] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United States
[2] Space Research Institute, Russian Academy of Science, Profsoyuznaya 84/32, Moscow 117997, Russian Federation
[3] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
[4] Department of Physics and Astronomy, Ohio University, Clippinger Lab 251B, Athens, OH 45701, United States
[5] Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611, United States
[6] Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 20450, MS-29, Stanford, CA 94309, United States - Source
The Astrophysical journal. 2008, Vol 679, Num 2, pp 1173-1180, 8 p ; 1 ; ref : 1/2 p
- 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
- Russian
- Author keyword
- dark matter galaxies: clusters: individual (IE 0657-56) ¯large-scale structure of universe methods: numerical
- Keyword (fr)
- Amas galaxies Galaxies en coalescence Matière sombre Méthode numérique Section efficace Simulation numérique Structure grande échelle
- Keyword (en)
- Galaxy clusters Merging galaxies Dark matter Numerical method Cross sections Digital simulation Large-scale structure
- Keyword (es)
- Galaxias en coalescencia Método numérico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20390080
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
10.1086/587859 
https://dx.doi.org/10.1086/587859
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