Spin alignment of dark matter haloes in the shells of the largest voids
- Author
- CUESTA, Antonio J1 ; BETANCORT-RIJO, Juan E2 3 ; GOTTLÖBER, Stefan4 ; PATIRI, Santiago G2 ; YEPES, Gustavo5 ; PRADA, Francisco1
[1] Instituto de Astrofisica de Andalucia (CSIC), Camino Bajo de Huétor 50, 18008 Granada, Spain
[2] Instituto de Astrofisica de Canarias, C/Via Ldctea s/n, 38200 La Laguna, Tenerife, Spain
[3] Universidad de La Laguna, Departamento de Astrofisica, Avda. Astrofisico Fco. Sdnchez s/n, 38200 La Laguna, Tenerife, Spain
[4] Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
[5] Universidad Autónoma de Madrid, Grupo de Astrofisica, 28049 Madrid, Spain - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 385, Num 2, pp 867-874, 8 p ; ref : 1/2 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- cosmology: theory dark matter galaxies: haloes large-scale structure of Universe methods: N-body simulations methods: statistical
- Keyword (fr)
- Alignement Corrélation Cosmologie Déplacement vers le rouge Galaxies spirales Halo galaxies Intensité Matière sombre Moment cinétique Méthode statistique Simulation numérique Structure grande échelle Système n corps
- Keyword (en)
- Alignment Correlations Cosmology Red shift Spiral galaxies Galaxy halo Intensity Dark matter Angular momentum Statistical method Digital simulation Large-scale structure N body system
- Keyword (es)
- Halo galaxia Intensidad Método estadístico Sistema n cuerpos
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20207199
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
10.1111/j.1365-2966.2008.12879.x 
https://dx.doi.org/10.1111/j.1365-2966.2008.12879.x
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