Baryons at the edge of the X-ray-brightest galaxy cluster

Science

Volumn 331, Issue 6024, 2011, Pages 1576-1579

  Simionescu, Aurora ^a   Allen, Steven W ^a   Mantz, Adam ^b   Werner, Norbert ^a   Takei, Yoh ^c   Morris, R Glenn ^a   Fabian, Andrew C ^d   Sanders, Jeremy S ^d   Nulsen, Paul E J ^e   George, Matthew R ^f   Taylor, Gregory B ^g,h  

^a STANFORD UNIVERSITY   (United States)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITY OF NEW MEXICO   (United States)

^h NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; COSMOLOGY; EXTRATERRESTRIAL MATTER; GAS; X-RAY;

ARTICLE; BARYON; COSMOS; ELECTRON; GALAXY CLUSTER; GAS; PHYSICS; PRIORITY JOURNAL; ROENTGEN SPECTROSCOPY; TEMPERATURE; X RAY;

EID: 79953158821     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1200331     Document Type: Article

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32. We thank P. Thomas and O. Young for kindly providing the simulation results shown in Fig. 4. Support for this work was provided by NASA through Einstein Postdoctoral Fellowship grants number PF9-00070 and PF8-90056 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. We acknowledge NASA grants NNX09AV64G and NNX10AR48G, issued through the Suzaku Guest Observer program, and grant NNX08AZ88G. The authors thank the Suzaku operation team and Guest Observer Facility, supported by JAXA and NASA. This work was supported in part by the U.S. Department of Energy under contract number DE-AC02-76SF00515. We also acknowledge the Grant-in-Aid for Scientific Research of the Ministry of Education, Culture, Sports, Science, and Technology of Japan (KAKENHI no. 22111513) and Chandra award GO0-11138B.