位置：成果数据库 > 会议 > 会议详情页
The kinematics and chemistry of the Sagittarius streams
  • 所属机构名称：北京大学
  • 会议名称：IAU Symposium 289
  • 时间：2013.2.2
  • 成果类型：会议
  • 相关项目：发射线气体星云的深度分光观测和三维数值模拟研究及相关原子参数计算
作者： Shi W.-B., Chen Y.-Q., Carrell K., Zhao G.|
同会议论文项目
发射线气体星云的深度分光观测和三维数值模拟研究及相关原子参数计算
期刊论文 30 会议论文 12
同项目会议论文
The properties of a large sample of low surface brightness galaxies from SDSS
Comparing six evolutionary population synthesis models
Stellar populations of local infrared-selected galaxies
Stellar Population Analysis on a Large Sample of Low Surface Brightness Galaxies
The stellar populations of host galaxies of supernovae
The [NII]/Hα calibration of the metallicity of galaxies from Te-based abundances
Plasma diagnostics for planetary nebulae and H II regions using the N II and O II optical recombinat
Very deep spectroscopy of the bright Saturn nebula NGC7009: The optical recombination spectrum and n
Atomic processes in planetary nebulae
[Fe III] emission lines in the planetary nebula NGC2392
Plasma diagnostics of emission-line galaxies in SDSS