Holdings: Amplification of magnetic fields in the centers of cluster cooling flows.

Amplification of magnetic fields in the centers of cluster cooling flows.

In 1990, Soker & Sarazin predicted that cooling Nows in clusters of galaxies would compress ambient intracluster magnetic Delds until the magnetic pressure becomes comparable to the local thermal pressure. Strong, centrally enhanced magnetic Delds were subsequently detected through Faraday rotation...

Bibliographic Details
Main Authors:	Godon, Patrick., Soker, Noam., White, Raymond III.
Format:	Villanova Faculty Authorship
Language:	English
Published:	1998
Online Access:	http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176423

Main Authors:

Godon, Patrick., Soker, Noam., White, Raymond III.

Format:

Villanova Faculty Authorship

Language:

English

Published:

1998

Online Access:

http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176423

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Amplification of magnetic fields in the centers of cluster cooling flows.

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Amplification of magnetic fields in the centers of cluster cooling flows.

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