查看“文献阅读”的源代码


==专题==
[[Documents on clusters of galaxies]]

[[size evolution]]

[[AGN的几何模型]]

[[银河系结构模型]]

==astro/ph==
[http://arxiv.org/abs/1308.4145] [[1308.4145]]

[http://arxiv.org/abs/1210.7815] [[1210.7815]]

[http://arxiv.org/abs/1209.4598] [[1209.4598]]

[http://arxiv.org/abs/1209.5748] [[1209.5748]]

[http://arxiv.org/abs/1208.5143] [[1208.5143]]

[http://arxiv.org/abs/1208.2584] [[1208.2584]]

[http://arxiv.org/abs/1208.2424] [[1208.2424]]

[[http://arxiv.org/abs/1208.2272] [[1208.2272]]

[http://arxiv.org/abs/1206.4063] [[1206.4063]]

[http://arxiv.org/abs/1206.4046] [[1206.4046]]

[http://arxiv.org/abs/1206.2679] [[1206.2679]] 

[http://arxiv.org/abs/1206.2642] [[1206.2642]]

[http://arxiv.org/abs/1204.0782] [[1204.0782]]

[http://arxiv.org/abs/1204.0793] [[1204.0793]]

[http://arxiv.org/abs/1203.4231] [[1203.4231]]

[http://arxiv.org/abs/1203.1641] [[1203.1641]]

IFU观测表明晕的质量很大，suggesting that dark matter halos may play a major role
in regulating the growth of the supermassive black holes.

arXiv:1203.1651:
-----------------------------
Advanced Camera for Surveys General Catalog (ACS-GC).
490,000 astronomical sources (stars + galaxies) ,r
edshifts (spectroscopic and photometric) for a considerable fraction
(~71%) of the imaging sample.
Includes color postage stamps, Galfit residual images, and photometry,
structural parameters, and redshifts combined into a single catalog.

arXiv:1203.1693
-----------------------------
Bar fraction和星系的颜色，质量有关，与是否AGN没关系。