搜索结果: 1-9 共查到“恒星与银河系 H-surface”相关记录9条 . 查询时间(0.142 秒)
Gyroscopic Pumping in the Solar Near-Surface Shear Layer
Gyroscopic Pumping Solar Near-Surface
2011/9/29
We use global and local helioseismic inversions to explore the prevailing dynamical balances in the solar Near-Surface Shear Layer (NSSL). The differential rotation and meridional circulation are inti...
A Correlation Between Surface Densities of Young Stellar Objects and Gas in Eight Nearby Molecular Clouds
Stellar Objects Gas Nearby Molecular Clouds
2011/9/28
We report the discovery and characterization of a power law correlation between the local surface densities of Spitzer-identified, dusty young stellar objects and the column density of gas (as traced ...
Surface-brightness fluctuations in stellar populations
Surface-brightness fluctuations stellar populations
2009/6/30
Surface-brightness fluctuations in stellar populations。
Numerical simulation of the surface flow of a companion Star in a semi-detached binary system and its application To galactic supersoft x-ray sources
companion Star semi-detached binary system x-ray sources
2009/6/17
Numerical simulation of the surface flow of a companion Star in a semi-detached binary system and its application To galactic supersoft x-ray sources。
Near-Infrared Surface Brightness Fluctuations as Diagnostics of Unresolved Stellar Populations
Near-Infrared Unresolved Stellar Populations Surface Brightness
2009/6/12
Near-Infrared Surface Brightness Fluctuations as Diagnostics of Unresolved Stellar Populations。
The Mass-Density Profiles of Low Surface Brightness Galaxies
Mass-Density Profiles Low Surface Brightness Galaxies
2009/6/11
The Mass-Density Profiles of Low Surface Brightness Galaxies。
Surface Brightness Profiles of Galactic Globular Clusters
Surface Brightness Profiles Galactic Globular Clusters
2009/6/9
Surface Brightness Profiles of Galactic Globular Clusters。
In an earlier analysis it was demonstrated that general relativity
gives higher values of surface tension in strange stars with quark
matter than neutron stars.We generate the modified Tolman–Oppenh...
Reviving a calculation made by Eddington in the 1920s, and using the most recent and comprehensive databases available on stars and galaxies, including more than 2,500,000 stars and around 20,000 gala...