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无编辑摘要 |
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[[星系的三维结构]] |
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[[文献：星系对和星系相互作用]] |
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[[文献：星系]] |
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[[文献：AGN]] |
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[[文献：scaling relation]] |
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[[文献：星系团]] |
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==Catalog== |
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*[http://www.atnf.csiro.au/people/Amy.Kimball/radiocat.shtml Unified Radio Catalog ] http://arxiv.org/abs/1401.1535 |
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*Catalog of Visually Classified Galaxies in the Local ($z\sim0.01$) Universe[http://arxiv.org/abs/1502.03545 arXiv:1502.03545] |
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:morphology catalog of 5840 galaxies in SDSS DR7. |
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==bar/bulge== |
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*1203.1693 [[Bar]] fraction和星系的颜色，质量有关，与是否AGN没关系。 |
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* arXiv:1409.5434 [[Galaxy Zoo]]: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2 < z < 1.0? |
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: bar跟AGN没关系 |
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*[arXiv:1606.04540]: Boxy/peanut bulges reduce gas inflow to the central kiloparsec |
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*2211.15681： bar区域SFR被抑制 |
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* 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 |
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==astro/ph== |
==astro/ph== |
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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]] |
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*arXiv:1502.02949: Galaxy rotation curves with [[log-normal density distribution]] |
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*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。 |
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*arXiv:1409.7388: The star formation history of galaxies in 3D: The [[CALIFA]] perspective |
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: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 |
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:[[STARTLIGHT]]拟合给出的dust的Tau_V和Sigma_SFR的关系可以重现KS定理 |
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*arXiv:1409.6791：The [[KMOS]]^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7 |
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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. |
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* arXiv:1409.5433 The Herschel view of the dominant mode of galaxy growth from z=4 to the present day |
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: 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 |
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* arXiv:1409.5468 The Star Formation Relation for Regions in the Galactic Plane: The Effect of Spatial Resolution |
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: 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。 |
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[http://arxiv.org/abs/1308.4145] [[1308.4145]] |
[http://arxiv.org/abs/1308.4145] [[1308.4145]] |
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[http://arxiv.org/abs/1208.5143] [[1208.5143]] |
[http://arxiv.org/abs/1208.5143] [[1208.5143]] |
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[http://arxiv.org/abs/1208.2584] [[1208.2584]] |
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[http://arxiv.org/abs/1208.2424] [[1208.2424]] |
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[[http://arxiv.org/abs/1208.2272] [[1208.2272]] |
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[http://arxiv.org/abs/1206.4063] [[1206.4063]] |
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[http://arxiv.org/abs/1206.4046] [[1206.4046]] |
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[http://arxiv.org/abs/1206.2679] [[1206.2679]] |
[http://arxiv.org/abs/1206.2679] [[1206.2679]] |
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[http://arxiv.org/abs/1206.2642] [[1206.2642]] |
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[http://arxiv.org/abs/1204.0782] [[1204.0782]] |
[http://arxiv.org/abs/1204.0782] [[1204.0782]] |
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[http://arxiv.org/abs/1203.1039] [[1203.1039]] |
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[http://arxiv.org/abs/1204.0793] [[1204.0793]] |
[http://arxiv.org/abs/1204.0793] [[1204.0793]] |
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[http://arxiv.org/abs/1203.4231] [[1203.4231]] |
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[http://arxiv.org/abs/1203.1641] [[1203.1641]] |
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[[Documents on clusters of galaxies]] |
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[http://arxiv.org/abs/1203.1651] [[1203.1651]] |
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[[size evolution]] |
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[http://arxiv.org/abs/1203.1693] [[1203.1693]] |
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[[AGN的几何模型]] |
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[[1203.1356]] |
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[[1203.1323]] |
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[[1203.0956]] |
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[[1203.0310]] |
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2024年9月23日 (一) 14:11的最新版本
专题
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: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。