Zobrazeno 1 - 10
of 411
pro vyhledávání: '"Dou Jing"'
Autor:
Dou, Jing, Peng, Yingjie, Gu, Qiusheng, Renzini, Alvio, Ho, Luis C., Mannucci, Filippo, Daddi, Emanuele, Zhang, Chengpeng, Li, Jiaxuan, Shi, Yong, Wang, Tao, Zhao, Dingyi, Lyu, Cheqiu, Li, Di, Yuan, Feng, Maiolino, Roberto, Gao, Yulong
The cold interstellar medium (ISM) as the raw material for star formation is critical to understanding galaxy evolution. It is generally understood that galaxies stop making stars when, in one way or another, they run out of gas. However, here we pro
Externí odkaz:
http://arxiv.org/abs/2409.03168
Autor:
Zhao, Dingyi, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Gallazzi, Anna R., Lyu, Cheqiu, Maiolino, Roberto, Dou, Jing, Gao, Zeyu, Gu, Qiusheng, Mannucci, Filippo, Mo, Houjun, Wang, Bitao, Wang, Enci, Wang, Kai, Wang, Yu-Chen, Xu, Bingxiao, Yuan, Feng, Zhu, Xingye
In $\Lambda$CDM cosmology, galaxies form and evolve in their host dark matter (DM) halos. Halo mass is crucial for understanding the halo-galaxy connection. The abundance matching (AM) technique has been widely used to derive the halo masses of galax
Externí odkaz:
http://arxiv.org/abs/2408.12442
Autor:
Gao, Zeyu, Peng, Yingjie, Wang, Kai, Ho, Luis C., Renzini, Alvio, Gallazzi, Anna R., Mannucci, Filippo, Mo, Houjun, Jing, Yipeng, Yang, Xiaohu, Wang, Enci, Zhao, Dingyi, Dou, Jing, Gu, Qiusheng, Lyu, Cheqiu, Maiolino, Roberto, Wang, Bitao, Wang, Yu-Chen, Xu, Bingxiao, Yuan, Feng, Zhu, Xingye
The spectral energy distribution (SED) of galaxies is essential for deriving fundamental properties like stellar mass and star formation history (SFH). However, conventional methods, including both parametric and non-parametric approaches, often fail
Externí odkaz:
http://arxiv.org/abs/2408.07749
Autor:
Lyu, Cheqiu, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Zhao, Dingyi, Mannucci, Filippo, Mo, Houjun, Wang, Kai, Wang, Bitao, Xu, Bingxiao, Dou, Jing, Gallazzi, Anna R., Gu, Qiusheng, Maiolino, Roberto, Wang, Enci, Yuan, Feng
The properties of the galaxies are tightly connected to their host halo mass and halo assembly history. Accurate measurement of the halo assembly history in observation is challenging but crucial to the understanding of galaxy formation and evolution
Externí odkaz:
http://arxiv.org/abs/2407.03409
Publikováno v:
E3S Web of Conferences, Vol 441, p 01019 (2023)
This paper introduces the technical routes and characteristics of four traditional adiponitrile production processes, including acrylonitrile dimerization method, butadiene method, adipic acid catalytic ammonification method and caprolactam method, w
Externí odkaz:
https://doaj.org/article/7fff640043ff4028b8317b23d484516f
Autor:
Lyu, Cheqiu, Peng, Yingjie, Jing, Yipeng, Yang, Xiaohu, Ho, Luis C., Renzini, Alvio, Wang, Bitao, Wang, Kai, Xu, Bingxiao, Zhao, Dingyi, Dou, Jing, Gu, Qiusheng, Maiolino, Roberto, Mannucci, Filippo, Yuan, Feng
The assembly of galaxies over cosmic time is tightly connected to the assembly of their host dark matter halos. We investigate the stellar mass growth history and the chemical enrichment history of central galaxies in SDSS-MaNGA. We find that the der
Externí odkaz:
http://arxiv.org/abs/2310.10733
Autor:
Gao, Yulong, Gu, Qiusheng, Liu, Guilin, Zhang, Hongxin, Shi, Yong, Dou, Jing, Li, Xiangdong, Kong, Xu
Publikováno v:
A&A 677, A179 (2023)
The physical mechanisms driving starbursts in dwarf galaxies are unclear, and the effects of mergers on star formation in these galaxies are still uncertain. We explore how the merger process affects star formation in metal-poor dwarf galaxies by ana
Externí odkaz:
http://arxiv.org/abs/2308.01128
Autor:
Shi, Jingjing, Peng, Yingjie, Diemer, Benedikt, Stevens, Adam R. H., Pillepich, Annalisa, Renzini, Alvio, Dou, Jing, Gao, Yu, Gu, Qiusheng, Ho, Luis C., Kong, Xu, Lagos, Claudia del P., Li, Di, Li, Jiaxuan, Maiolino, Roberto, Mannucci, Filippo, Xie, Lizhi, Zhang, Chengpeng
Black hole feedback has been widely implemented as the key recipe to quench star formation in massive galaxies in modern semi-analytic models and hydrodynamical simulations. As the theoretical details surrounding the accretion and feedback of black h
Externí odkaz:
http://arxiv.org/abs/2202.01376
Publikováno v:
In Carbon Trends June 2024 15
Autor:
Dou, Jing, Peng, Yingjie, Renzini, Alvio, Ho, Luis C., Mannucci, Filippo, Daddi, Emanuele, Gao, Yu, Maiolino, Roberto, Zhang, Chengpeng, Gu, Qiusheng, Li, Di, Lilly, Simon J., Pan, Zhizheng, Yuan, Feng, Zheng, Xianzhong
In Dou et al. (2021), we introduced the Fundamental Formation Relation (FFR), a tight relation between specific SFR (sSFR), H$_2$ star formation efficiency (SFE$_{\rm H_2}$), and the ratio of H$_2$ to stellar mass. Here we show that atomic gas HI doe
Externí odkaz:
http://arxiv.org/abs/2104.12794