Diffuse Extreme-Ultraviolet Emission from the Coma Cluster: Evidence for Rapidly Cooling Gases at Submegakelvin Temperatures-Reference-Cited by-同舟云学术

Diffuse Extreme-Ultraviolet Emission from the Coma Cluster: Evidence for Rapidly Cooling Gases at Submegakelvin Temperatures

Author:

Lieu Richard¹,Mittaz Jonathan P. D.²,Bowyer Stuart³,Breen Jeffrey O.⁴,Lockman Felix J.⁵,Murphy Edward M.⁴,Hwang Chorng-yuan³

Affiliation:

1. R. Lieu, Department of Physics, University of Alabama, Huntsville, AL 35899, USA.

2. J. P. D. Mittaz, Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK.

3. S. Bowyer and C.-y. Hwang, Center for Extreme Ultraviolet Astrophysics, University of California, Berkeley, CA 94720, USA.

4. J. O. Breen and E. M. Murphy, Astronomy Department, University of Virginia, Post Office Box 3818, Charlottesville, VA 22903, USA.

5. F. J. Lockman, National Radio Astronomy Observatory, Green Bank, WV 24944, USA.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference27 articles.

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2. Fabian A. C., Arnaud K. A., Bautz M. W., Tawara Y., ibid. 436, L63 (1994).

3. Briel U. G., Henry J. P., Böhringer H., Astron. Astrophys. 259, L31 (1992).

4. See the High Energy Astrophysics Archive available at http://heasarc.gsfc.nasa.gov/docs/rosat/archive.html.

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