Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Crater 2: An Extremely Cold Dark Matter Halo

  • Authors: Nelson Caldwell, Matthew G. Walker, Mario Mateo, Edward W. Olszewski, Sergey Koposov, Vasily Belokurov, Gabriel Torrealba, Alex Geringer-Sameth, and Christian I. Johnson

2017 The Astrophysical Journal 839 20.

  • Provider: AAS Journals

Caption: Figure 6.

Velocity dispersion vs. halflight radius, for the population of dwarf spheroidals plotted in Figure 5 (excluding those for which the vertical errorbar is >100%). Overplotted is the scaling relation ﹩{ \mathcal V }/(\mathrm{km}\,{{\rm{s}}}^{-1})=\sqrt{{R}_{{\rm{h}}}/\mathrm{pc}}﹩, where ﹩{ \mathcal V }\equiv \sqrt{3}{\sigma }_{{v}_{\mathrm{los}}}﹩ (McGaugh et al. 2007; Walker et al. 2010; Walker & Loeb 2014).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions