Image Details

Choose export citation format:

Mass Distribution in Galaxy Cluster Cores

  • Authors: M. T. Hogan, B. R. McNamara, F. Pulido, P. E. J. Nulsen, H. R. Russell, A. N. Vantyghem, A. C. Edge, and R. A. Main

2017 The Astrophysical Journal 837 51.

  • Provider: AAS Journals

Caption: Figure 4.

Percentage error introduced to resulting projected (left) and deprojected (right) cooling time profiles when a single temperature is assumed across the central ∼20 kpc, achieved here by first fitting to coarsely binned spectra and then forcing the resulting temperatures on the more finely binned spectra (see text for more details). Errors are typically <10% in projection, though the effect is exacerbated after deprojection.

Other Images in This Article
Copyright and Terms & Conditions