期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 422, 期 1, 页码 L62-L66出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1745-3933.2012.01237.x
关键词
galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: formation
资金
- PRIN MIUR
- ERC [ERC-2010-AdG-26107-EARLY]
- ASI-Uni. Bologna-Astronomy Dept. [I/039/10/0]
- [PRIN MIUR 2008]
We present the analysis of a large sample of early-type galaxies (ETGs) at 0 < z < 3 aimed at tracing the cosmic evolution of their size and compare it with a model of pure dissipationless (dry) merging in the Lambda cold dark matter (Lambda CDM) framework. The effective radius R-e depends on stellar mass M as R-e(M) alpha M-alpha with alpha similar to 0.5 at all redshifts. The redshift evolution of the mass- or SDSS-normalized size can be reproduced as alpha(1 + z)(beta) with beta similar to -1, with the most massive ETGs possibly showing the fastest evolutionary rate (beta similar to -1.4). This size evolution slows down significantly to beta similar to -0.6 if the ETGs at z > 2 are removed from the sample, suggesting an accelerated increase of the typical sizes at z > 2, especially for the ETGs with the largest masses. A pure dry merging Lambda CDM model is marginally consistent with the average size evolution at 0 < z < 1.7, but predicts descendants too compact for z > 2 progenitor ETGs. This opens the crucial question on what physical mechanism can explain the accelerated evolution at z > 2, or whether an unclear observational bias is partly responsible for that.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据