The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape
- Author
- MUNOZ-CUARTAS, J. C1 ; MACCIO, A. V2 ; GOTTLÖBER, S1 ; DUTTON, A. A3
[1] Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
[2] Max-Planck-Institut Für Astronomie, Köningstuhl 17, 69117 Heidelberg, Germany
[3] Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada - Source
Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 411, Num 1, pp 584-594, 11 p ; ref : 1/2 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
- English
- Author keyword
- cosmology: theory dark matter galaxies: haloes gravitation methods: numerical
- Keyword (fr)
- Corrélation Cosmologie Déplacement vers le rouge Effondrement Etude sur modèle Gravitation Halo galaxies Loi puissance Matière sombre froide Matière sombre Modèle sphérique Méthode numérique Simulation numérique Système n corps
- Keyword (en)
- Correlations Cosmology Red shift Collapse Model study Gravitation Galaxy halo Power law Cold dark matter Dark matter Spherical model Numerical method Digital simulation N body system
- Keyword (es)
- Desmoronamiento Estudio sobre modelo Halo galaxia Ley poder Materia oscura fría Método numérico Sistema n cuerpos
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 23764153
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
Access to the document
Install on your browser
DOI
10.1111/j.1365-2966.2010.17704.x 
https://dx.doi.org/10.1111/j.1365-2966.2010.17704.x
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:32:\"10.1111\/j.1365-2966.2010.17704.x\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:9:\"\u0000*\u0000jtitle\";s:57:\"Monthly notices of the Royal Astronomical Society (Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Mon. not. R. Astron. Soc. (Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2011\";s:9:\"\u0000*\u0000volume\";s:3:\"411\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:3:\"584\";s:8:\"\u0000*\u0000epage\";s:3:\"594\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0035-8711\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:13:\"MUNOZ-CUARTAS\";s:10:\"\u0000*\u0000aufirst\";s:4:\"J. C\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:12:\"MACCIO, A. V\";i:1;s:13:\"GOTTL\u00d6BER, S\";i:2;s:12:\"DUTTON, A. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"MNRAA4\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:8:\"\u0000*\u0000place\";s:10:\"Malden, MA\";s:6:\"\u0000*\u0000pub\";s:15:\"Wiley-Blackwell\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"11\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Panist access
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:32:\"10.1111\/j.1365-2966.2010.17704.x\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:9:\"\u0000*\u0000jtitle\";s:57:\"Monthly notices of the Royal Astronomical Society (Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Mon. not. R. Astron. Soc. (Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2011\";s:9:\"\u0000*\u0000volume\";s:3:\"411\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:3:\"584\";s:8:\"\u0000*\u0000epage\";s:3:\"594\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0035-8711\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:13:\"MUNOZ-CUARTAS\";s:10:\"\u0000*\u0000aufirst\";s:4:\"J. C\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:12:\"MACCIO, A. V\";i:1;s:13:\"GOTTL\u00d6BER, S\";i:2;s:12:\"DUTTON, A. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"MNRAA4\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:8:\"\u0000*\u0000place\";s:10:\"Malden, MA\";s:6:\"\u0000*\u0000pub\";s:15:\"Wiley-Blackwell\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"11\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Istex access
"O:16:\"UnpaywallOpenUrl\":35:{s:8:\"\u0000*\u0000email\";s:27:\"assistance-portail@inist.fr\";s:6:\"\u0000*\u0000fmt\";N;s:6:\"\u0000*\u0000doi\";s:32:\"10.1111\/j.1365-2966.2010.17704.x\";s:6:\"\u0000*\u0000pii\";N;s:7:\"\u0000*\u0000pmid\";N;s:9:\"\u0000*\u0000atitle\";N;s:9:\"\u0000*\u0000jtitle\";N;s:9:\"\u0000*\u0000stitle\";N;s:7:\"\u0000*\u0000date\";N;s:9:\"\u0000*\u0000volume\";N;s:8:\"\u0000*\u0000issue\";N;s:8:\"\u0000*\u0000spage\";N;s:8:\"\u0000*\u0000epage\";N;s:8:\"\u0000*\u0000pages\";N;s:7:\"\u0000*\u0000issn\";N;s:8:\"\u0000*\u0000eissn\";N;s:9:\"\u0000*\u0000aulast\";N;s:10:\"\u0000*\u0000aufirst\";N;s:9:\"\u0000*\u0000auinit\";N;s:10:\"\u0000*\u0000auinitm\";N;s:5:\"\u0000*\u0000au\";N;s:9:\"\u0000*\u0000aucorp\";N;s:7:\"\u0000*\u0000isbn\";N;s:8:\"\u0000*\u0000coden\";N;s:8:\"\u0000*\u0000genre\";N;s:7:\"\u0000*\u0000part\";N;s:9:\"\u0000*\u0000btitle\";N;s:8:\"\u0000*\u0000title\";N;s:8:\"\u0000*\u0000place\";N;s:6:\"\u0000*\u0000pub\";N;s:10:\"\u0000*\u0000edition\";N;s:9:\"\u0000*\u0000tpages\";N;s:9:\"\u0000*\u0000series\";N;s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";N;}"
Unpaywall access
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:32:\"10.1111\/j.1365-2966.2010.17704.x\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:9:\"\u0000*\u0000jtitle\";s:57:\"Monthly notices of the Royal Astronomical Society (Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Mon. not. R. Astron. Soc. (Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2011\";s:9:\"\u0000*\u0000volume\";s:3:\"411\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:3:\"584\";s:8:\"\u0000*\u0000epage\";s:3:\"594\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0035-8711\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:13:\"MUNOZ-CUARTAS\";s:10:\"\u0000*\u0000aufirst\";s:4:\"J. C\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:12:\"MACCIO, A. V\";i:1;s:13:\"GOTTL\u00d6BER, S\";i:2;s:12:\"DUTTON, A. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"MNRAA4\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:8:\"\u0000*\u0000place\";s:10:\"Malden, MA\";s:6:\"\u0000*\u0000pub\";s:15:\"Wiley-Blackwell\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"11\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Europe PubMed Central access
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:32:\"10.1111\/j.1365-2966.2010.17704.x\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:9:\"\u0000*\u0000jtitle\";s:57:\"Monthly notices of the Royal Astronomical Society (Print)\";s:9:\"\u0000*\u0000stitle\";s:33:\"Mon. not. R. Astron. Soc. (Print)\";s:7:\"\u0000*\u0000date\";s:4:\"2011\";s:9:\"\u0000*\u0000volume\";s:3:\"411\";s:8:\"\u0000*\u0000issue\";s:1:\"1\";s:8:\"\u0000*\u0000spage\";s:3:\"584\";s:8:\"\u0000*\u0000epage\";s:3:\"594\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0035-8711\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:13:\"MUNOZ-CUARTAS\";s:10:\"\u0000*\u0000aufirst\";s:4:\"J. C\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:3:{i:0;s:12:\"MACCIO, A. V\";i:1;s:13:\"GOTTL\u00d6BER, S\";i:2;s:12:\"DUTTON, A. A\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:6:\"MNRAA4\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:91:\"The redshift evolution of A cold dark matter halo parameters: concentration, spin and shape\";s:8:\"\u0000*\u0000place\";s:10:\"Malden, MA\";s:6:\"\u0000*\u0000pub\";s:15:\"Wiley-Blackwell\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:2:\"11\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
arXiv access
