REVISED MASS-TO-LIGHT RATIOS FOR NEARBY GALAXY GROUPS AND CLUSTERS
We present a detailed investigation of the cluster stellar mass-to-light (M*/L) ratio and cumulative stellar masses, derived on a galaxy-by-galaxy basis, for 12 massive (M [subscript 500] ~ 10[superscript 14]-10[superscript 15] M [subscript ☉]), nearby clusters with available optical imaging data fr...
| Main Authors: | , , |
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| 格式: | 文件 |
| 语言: | en_US |
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IOP Publishing
2015
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| 在线阅读: | http://hdl.handle.net/1721.1/96792 |