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Cooling Flows in Clusters and Galaxies
Tallenna

Cooling Flows in Clusters and Galaxies

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.
Toimittaja
A.C. Fabian
Painos
Softcover reprint of the original 1st ed. 1988
ISBN
9789401078283
Kieli
englanti
Paino
310 grammaa
Julkaisupäivä
12.10.2011
Kustantaja
Springer
Sivumäärä
406