ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ONY-MSCALING RELATIONS-Reference-Cited by-同舟云学术

ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ONY-MSCALING RELATIONS

Published:2012-09-27 Issue:2 Volume:758 Page:74
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Battaglia N.,Bond J. R.,Pfrommer C.,Sievers J. L.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/758/i=2/a=74/pdf

Reference115 articles.

1. Fundamental Plane of Sunyaev‐Zel’dovich Clusters

2. Fundamental differences between SPH and grid methods

3. The shape of dark matter haloes: dependence on mass, redshift, radius and formation

4. X-RAY PROPERTIES OF THE FIRST SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTER SAMPLE FROM THE SOUTH POLE TELESCOPE

5. The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and theYSZ–M500relation

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