Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Tidal Disruption of Dark Matter Halos around Proto–Globular Clusters

  • Authors: Takayuki R. Saitoh, Jin Koda, Takashi Okamoto, Keiichi Wada, and Asao Habe

Saitoh et al. 2006 The Astrophysical Journal 640 22.

  • Provider: AAS Journals

Caption: Fig. 10.

Evolution of masses of the reference clump and mb/mtot of the clump. Thin solid, dashed, dot‐dashed, and dotted lines indicate the masses of baryons, gas, stars, and dark matter in the clump, respectively. The thick solid line shows the evolution of mb/mtot of the clump.

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
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions