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The Mass of Abell 1060 and AWM 7 from Spatially Resolved X‐Ray Spectroscopy: Variations in Baryon Fraction

  • Authors: M. Loewenstein and R. F. Mushotzky

Loewenstein & Mushotzky 1996 The Astrophysical Journal Letters 471 L83.

  • Provider: AAS Journals

Caption: Fig. 1.

(a) Projected, emission‐averaged, model temperature distribution superimposed on the 90% confidence limits from ASCA (error bars) for A1060. The best‐fit mass model, adark = 325 kpc (solid line); the most compact acceptable mass model, adark = 150 kpc (dotted line); and the most diffuse acceptable mass model—adark = 900 kpc (dashed line) are indicated. (b) Same as (a) but for AWM 7 with adark = 300, 100, and 650 kpc for the best‐fit, most compact, and most diffuse dark matter models, respectively.

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