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The 21-cm absorption line in NGC1275

✍ Scribed by EKERS, R. D.; VAN DER HULST, J. M.; MILEY, G. K.


Book ID
109701880
Publisher
Nature Publishing Group
Year
1976
Tongue
English
Weight
224 KB
Volume
262
Category
Article
ISSN
0028-0836

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## Abstract NGC 1275, the central galaxy of the Perseus cluster, contains a remarkable cool ISM. This gas is arrayed in a series of filaments extending over 30 kpc with an extension of 70 kpc to the north. These emit substantial cooling line radiation from HII, a hot H~2~ zone, and CO in a cool mol