Publisher： Edp Sciences
E-ISSN： 1638-1963|20|issue|25-28
ISSN： 1633-4760
Source： EAS Publications Series, Vol.20, Iss.issue, 2006-05, pp. : 25-28
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Using high resolution DM simulations we study the shape of dark matter halos. Halos become more spherical with decreasing mass. This trend is even more pronounced for the inner part of the halo. Angular momentum and shape are correlated. The angular momenta of neighboring halos are correlated.
Related content
Access to resources
Recommend
The dark matter halo shape of edge-on disk galaxies
By O'Brien J. C. Freeman K. C. van der Kruit P. C.
Astronomy & Astrophysics, Vol. 515, Iss. issue, 2010-06 ,pp. :
The dark matter halo shape of edge-on disk galaxies
By O'Brien J. C. Freeman K. C. van der Kruit P. C.
Astronomy & Astrophysics, Vol. 515, Iss. issue, 2010-06 ,pp. :
The dark matter halo shape of edge-on disk galaxies
By O'Brien J. C. Freeman K. C. van der Kruit P C. Bosma A.
Astronomy & Astrophysics, Vol. 515, Iss. issue, 2010-06 ,pp. :
The dark matter halo shape of edge-on disk galaxies
By O'Brien J. C. Freeman K. C. van der Kruit P. C.
Astronomy & Astrophysics, Vol. 515, Iss. issue, 2010-06 ,pp. :