101. A good mass proxy for galaxy clusters with XMM-Newton
- Author
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Zhao, Hai-Hui, Jia, Shu-Mei, Chen, Yong, Li, Cheng-Kui, Song, Li-Ming, and Xie, Fei
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We use a sample of 39 galaxy clusters at redshift z < 0.1 observed by XMM-Newton to investigate the relations between X-ray observables and total mass. Based on central cooling time and central temperature drop, the clusters in this sample are divided into two groups: 25 cool core clusters and 14 non-cool core clusters, respectively. We study the scaling relations of Lbol-M500, M500-T, M500-Mg and M500-YX, and also the influences of cool core on these relations. The results show that the M500-YX relation has a slope close to the standard self-similar value, has the smallest scatter and does not vary with the cluster sample. Moreover, the M500-YX relation is not affected by the cool core. Thus, the parameter of YX may be the best mass indicator., Comment: ApJ Accepted, 25 pages, 7 figures
- Published
- 2013
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