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==专题==
[[星系的三维结构]]

[[文献：星系对和星系相互作用]]

[[文献：星系]]

[[文献：AGN]]

[[文献：scaling relation]]

[[文献：星系团]]

[[银河系结构模型]]

==Catalog==
*[http://www.atnf.csiro.au/people/Amy.Kimball/radiocat.shtml Unified Radio Catalog ] http://arxiv.org/abs/1401.1535

*Catalog of Visually Classified Galaxies in the Local ($z\sim0.01$) Universe[http://arxiv.org/abs/1502.03545 arXiv:1502.03545]
:morphology catalog of 5840 galaxies in SDSS DR7.


==bar/bulge==
*1203.1693 [[Bar]] fraction和星系的颜色，质量有关，与是否AGN没关系。
* 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:1606.04540]: Boxy/peanut bulges reduce gas inflow to the central kiloparsec
*2211.15681： bar区域SFR被抑制
* 2303.11441： fast bars live in baryon-dominated discs, whereas slow bars experienced a strong drag from the dynamical friction due to a dense DM halo

==astro/ph==
==astro/ph==
arXiv:1509.0579 compact group 中的星系的恒星形成被抑制了，与分子氢气体被加热有关 [[MOHEG]]
*arXiv:1502.02949: Galaxy rotation curves with [[log-normal density distribution]]

*arXiv:1412.7225： 星系的速度弥散度的测量对晚型星系来说与倾角有关。

*arXiv:1409.7388: The star formation history of galaxies in 3D: The [[CALIFA]] perspective
:在pxiel级别上，Halpha不一定是好的SFR的指针,而[[STARTLIGHT]]拟合给出的SFR没有改限制
:[[STARTLIGHT]]拟合给出的dust的Tau_V和Sigma_SFR的关系可以重现KS定理

*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:1409.5468 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。
[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/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/1203.1039] [[1203.1039]]

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

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

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

[http://arxiv.org/abs/1203.1651] [[1203.1651]]

[http://arxiv.org/abs/1203.1693] [[1203.1693]]

[[1203.1356]]

[[1203.1323]]

[[1203.0956]]

[[1203.0310]]

2024年9月23日 (一) 14:11的最新版本

专题

星系的三维结构

文献：星系对和星系相互作用

文献：星系

文献：AGN

文献：scaling relation

文献：星系团

银河系结构模型

Catalog

  • Catalog of Visually Classified Galaxies in the Local ($z\sim0.01$) UniversearXiv:1502.03545
morphology catalog of 5840 galaxies in SDSS DR7.


bar/bulge

  • 1203.1693 Bar fraction和星系的颜色，质量有关，与是否AGN没关系。
  • 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:1606.04540]: Boxy/peanut bulges reduce gas inflow to the central kiloparsec
  • 2211.15681： bar区域SFR被抑制
  • 2303.11441： fast bars live in baryon-dominated discs, whereas slow bars experienced a strong drag from the dynamical friction due to a dense DM halo

astro/ph

arXiv:1509.0579 compact group 中的星系的恒星形成被抑制了，与分子氢气体被加热有关 MOHEG

  • arXiv:1412.7225： 星系的速度弥散度的测量对晚型星系来说与倾角有关。
  • arXiv:1409.7388: The star formation history of galaxies in 3D: The CALIFA perspective
在pxiel级别上，Halpha不一定是好的SFR的指针,而STARTLIGHT拟合给出的SFR没有改限制
STARTLIGHT拟合给出的dust的Tau_V和Sigma_SFR的关系可以重现KS定理
  • 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:1409.5468 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

取自“http://202.127.29.3/~shen/wiki/index.php?title=文献阅读&oldid=4146”