搜索结果: 1-8 共查到“恒星与银河系 Probing”相关记录8条 . 查询时间(0.085 秒)
Probing the Microscopic with the Macroscopic: from Properties of Star Cluster Systems to Properties of Cluster-Forming Regions
Macroscopic: Properties Cluster Systems Cluster-Forming Regions
2011/10/11
To understand how systems of star clusters have reached their presently observed properties constitutes a powerful probe into the physics of cluster formation, without needing to resort to high spatia...
Probing cluster formation under extreme conditions: massive star clusters in blue compact galaxies
galaxies: starburst - galaxies: star clusters: general - galaxies: irregular- galaxies:star formation
2011/9/27
The numerous and massive young star clusters in blue compact galaxies (BCGs) are used to investigate the properties of their hosts. We test whether BCGs follow claimed relations between cluster popula...
Probing bulk viscous matter-dominated models with Gamma-ray bursts
Probing viscous matter-dominated Gamma-ray bursts
2011/9/27
In this paper we extend the range of consistency of a constant bulk viscosity model to redshifts up to $z\sim 8.1$. In this model the dark sector of the cosmic substratum is a viscous fluid with press...
Probing the Cores of Radio Jets through Interstellar Scintillation
Radio Jets Interstellar Scintillation
2009/7/1
Probing the Cores of Radio Jets through Interstellar Scintillation。
Probing structure and populations of our Galaxy using the kinematics of old stars. II
Probing structure kinematics of old stars Galaxy
2009/6/30
Probing structure and populations of our Galaxy using the kinematics of old stars. II。
Probing structure and populations of our Galaxy using the kinematics of old stars. I
Probing structure kinematics of old stars Galaxy
2009/6/30
Probing structure and populations of our Galaxy using the kinematics of old stars. I。
Probing galactic structure with musyc。
Fuse Observations of the Cygnus Loop：Probing Shock-Cloud Interactions
Cygnus Loop Shock-Cloud Interactions
2009/6/16
Fuse Observations of the Cygnus Loop：Probing Shock-Cloud Interactions。