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Home › Buoyant Bubbles in Galaxy Clusters ›

Inflated, Unmagnetized Bubbles in Tangled, Strong Ambient Fields (FIG 7)

Submitted by sean on Mon, 01/12/2009 - 13:17

Volume renderings of the passive mass fraction for inflated bubbles in tangled ambient fields. Light colors represent bubble material and dark represent the ICM.

TBS-I Model:

TLS-I Model:

‹ Inflated, Unmagnetized Bubbles in Various Environments (FIG 4) up Comparison of Magnetized and Unmagnetized Bubbles (FIG 8) ›

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University of Minnesota :: Minnesota Institute of Astrophysics
Contact :: Tom Jones :: twj@msi.umn.edu