Re-examination of the hubble constant from the Sunyaev-Zel'dovich effect: Implication for cosmological parameters

被引:18
作者
Kobayashi, S
Sasaki, S
Suto, Y
机构
[1] UNIV TOKYO, DEPT PHYS, SCH SCI, BUNKYO KU, TOKYO 113, JAPAN
[2] TOKYO METROPOLITAN UNIV, DEPT PHYS, HACHIOJI, TOKYO 19203, JAPAN
[3] UNIV TOKYO, SCH SCI, RES CTR EARLY UNIVERSE, BUNKYO KU, TOKYO 113, JAPAN
关键词
cosmology; galaxies; clusters of; radio sources; extended; X-rays; sources;
D O I
10.1093/pasj/48.6.L107
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We performed a systematic and comprehensive estimate of the Hubble constant Ho via the Sunyaev-Zel'dovich temperature decrement and X-ray measurements for clusters up to redshift z of 0.541, paying particular attention to its dependence on the density parameter Omega(0), and the cosmological constant lambda(0). The resulting values of H-0 are largely consistent with that derived from the Cepheid distance for nearby galaxies. We discuss how the angular diameter distance d(A) vs. z diagram from accurate SZ measurements of high-z clusters is dependent on the values of Omega(0) and lambda(0).
引用
收藏
页码:L107 / L111
页数:5
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