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The Perseus Cluster
Author(s) -
W. M. Smart,
A. Ali
Publication year - 1940
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/100.7.560
Subject(s) - physics , astrophysics , cluster (spacecraft) , brightest cluster galaxy , astronomy , galaxy cluster , galaxy , computer science , programming language
respectively. (Credit: NASA/CXC/Stanford/I.Zhuravleva et al Caption: Chandra observations of the Perseus and Virgo galaxy clusters have provided direct evidence that turbulence is helping to prevent stars from forming there. These new results could answer a long-standing question about how these galaxy clusters keep their enormous reservoirs of hot gas from cooling down to form stars. Scientists targeted Perseus and Virgo because they are both extremely large and relatively bright, thus providing an opportunity to see details that would be very difficult to detect in other clusters.

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