Comparisons between Isothermal and NFW Mass Profiles for Strong-Lensing Galaxy Clusters

Comparisons between Isothermal and NFW Mass Profiles for Strong-Lensing Galaxy ClustersDOI: info:10.1086/590049v. 68570–82
Shu, Chenggang, Zhou, Binglu, Bartelmann, Matthias, Comerford, Julia M., Huang, J. -S, and Mellier, Yannick. 2008. "Comparisons between Isothermal and NFW Mass Profiles for Strong-Lensing Galaxy Clusters." The Astrophysical Journal, 685 70–82. https://doi.org/10.1086/590049.
ID: 74461
Type: article
Keywords: SAO