文献阅读

专题

文献：星系

文献：AGN

文献：scaling relation

文献：星系团

银河系结构模型

Catalog

Unified Radio Catalog http://arxiv.org/abs/1401.1535

astro/ph

• arXiv:1409.6791：The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7

For rotation-dominated disks, the average intrinsic velocity dispersion decreases by a factor of two from 50 km/s at z~2.3 to 25 km/s at z~0.9 while the rotational velocities at the two redshifts are comparable. Combined withexisting results spanning z~0-3, disk velocity dispersions follow an approximate (1+z) evolution that is consistent with the dependence of velocity dispersion on gas fractions predicted by marginally-stable disk theory.

• arXiv:1409.5433 The Herschel view of the dominant mode of galaxy growth from z=4 to the present day

大部分宇宙中的恒星形成都是早期的，而且是MAIN SEQUENCE形式的，不是MERGE的

• arXiv:1409.5434 Galaxy Zoo: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2 < z < 1.0?

bar跟AGN没关系

• arXiv:1409.5468 The Star Formation Relation for Regions in the Galactic Plane: The Effect of Spatial Resolution

似乎在不同尺度（还是小尺度）上，恒星形成和分子密度还是线性的关系，和Kenicutt law不太一样。

[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] 1203.1039

[15] 1204.0793

[16] 1203.4231

[17] 1203.1641

[18] 1203.1651

[19] 1203.1693

1203.1356

1203.1323

1203.0956

1203.0310