## 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
On the Structure of the Perseus Cluster of Galaxies
β Scribed by F. W. Baier
- Publisher
- John Wiley and Sons
- Year
- 1984
- Tongue
- English
- Weight
- 608 KB
- Volume
- 305
- Category
- Article
- ISSN
- 0004-6337
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