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Cooling Flows in Clusters and Galaxies
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Cooling Flows in Clusters and Galaxies

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X-ray astronomers discovered the diffuse gas in clusters of galaxies about 20 years ago. It was later realized that the central gas density in some clusters, and in elliptical galaxies, is so high that radiative cooling is a significant energy loss.
Redaktör
A.C. Fabian
Upplaga
Softcover reprint of the original 1st ed. 1988
ISBN
9789401078283
Språk
Engelska
Vikt
310 gram
Utgivningsdatum
2011-10-12
Förlag
Springer
Sidor
406