Magnetic support of the optical emission line filaments in NGC 1275
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Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/nature07169.pdf
Reference20 articles.
1. Kent, S. M. & Sargent, W. L. W. Ionization and excitation mechanisms in the filaments around NGC 1275. Astrophys. J. 230, 667–680 (1979)
2. Conselice, C. J., Gallagher, J. S. & Wyse, R. F. G. On the nature of the NGC 1275 system. Astron. J. 122, 2281–2300 (2001)
3. Hatch, N. A., Crawford, C. S., Fabian, A. C. & Johnstone, R. M. Detections of molecular hydrogen in the outer filaments of NGC1275. Mon. Not. R. Astron. Soc. 358, 765–773 (2005)
4. Hatch, N. A., Crawford, C. S., Johnstone, R. M. & Fabian, A. C. On the origin and excitation of the extended nebula surrounding NGC1275. Mon. Not. R. Astron. Soc. 367, 433–448 (2006)
5. Fabian, A. C. et al. The relationship between the optical Hα filaments and the X-ray emission in the core of the Perseus cluster. Mon. Not. R. Astron. Soc. 344, L48–L52 (2003)
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