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

[[size evolution]]

[[AGN的几何模型]]

[[银河系结构模型]]

==astro/ph==
==astro/ph==
[http://arxiv.org/abs/1308.4145] [[1308.4145]]
[http://arxiv.org/abs/1308.4145] [[1308.4145]]
第30行: 第40行:
[http://arxiv.org/abs/1203.4231] [[1203.4231]]
[http://arxiv.org/abs/1203.4231] [[1203.4231]]


[http://arxiv.org/abs/1203.1641] [[1203.1641]]
==专题==
[[Documents on clusters of galaxies]]


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


arXiv:1203.1651:
[[AGN的几何模型]]
-----------------------------
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
[[银河系结构模型]]
-----------------------------
Bar fraction和星系的颜色,质量有关,与是否AGN没关系。

2013年12月19日 (四) 03:15的版本

专题

Documents on clusters of galaxies

size evolution

AGN的几何模型

银河系结构模型

astro/ph

[1] 1308.4145

[2] 1210.7815

[3] 1209.4598

[4] 1209.5748

[5] 1208.5143

[6] 1208.2584

[7] 1208.2424

[[8] 1208.2272

[9] 1206.4063

[10] 1206.4046

[11] 1206.2679

[12] 1206.2642

[13] 1204.0782

[14] 1204.0793

[15] 1203.4231

[16] 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。