位置：成果数据库 > 会议 > 会议详情页
What Causes the Abundance Gradient and its Evolution along the Galaxy Disk?
  • 所属机构名称：中国科学院上海天文台
  • 会议名称：The Eighth Pacific Rim Conference on Stellar Astrophysics: A Tribute to Kam-Ching Leung ASP Conferen
  • 成果类型：会议
  • 相关项目：星系化学演化－从高红移吸收体星系到近邻盘状星系
作者： Hou|L.|J. L.|Fu|J.|Chang|R. X.|Yin|J.|Chen|
同会议论文项目
星系化学演化－从高红移吸收体星系到近邻盘状星系
期刊论文 60 会议论文 16
同项目会议论文
Properties and chemical evolution of the M31 disk: Comparison with the Milky Way
Inclination-dependent LF of disc galaxies as a constraint of dust extinction law
Constrain the stellar population gradient of elliptical galaxies with SED
Photometric Properties of LBGsa at z ~ 1
Galactic Open Clusters and the LOCS Project
The Impacts of Continuous Infall, Outflow and Star Formation on the Chemical Evolution of Galaxies
Galaxy Evolution: Infrared to Millimeter Wavelength Perspective
What Causes the Abundance Gradient and its Evolution along the Galaxy Disk?
Effect of Galactic Wind on the Chemical Evolution of Galaxies
Using L dwarfs with distances to test models
What Causes the Abundance Gradient and its Evolution along the Galaxy Disk?
What Causes the Abundance Gradient and its Evolution along the Galaxy Disk?
Dark Matter Annihilation and the Cusp Problem
Modeling Damped Lyman-α Systems at z? 3
The Galactic Structure and Stellar Population in the CFHTLS Wide Fields