搜索结果: 106-120 共查到“天文学 dark matter”相关记录125条 . 查询时间(0.173 秒)
Dark Matter in Dwarf Spheroidal Galaxies。
The phase-space structure of CDM halos and dark-matter direct detection experiments
phase-space structure dark-matter direct CDM halos
2009/6/11
The phase-space structure of CDM halos and dark-matter direct detection experiments。
Low mass dark matter halos in voids。
The structure of halos in Self-Interacting Cold Dark Matter models
halos Self-Interacting Cold Dark Matter models
2009/6/11
The structure of halos in Self-Interacting Cold Dark Matter models。
Dark Matter in late-type galaxies。
Formation and Evolution of Self-Interacting Dark Matter Halos
Self-Interacting Dark Matter Halos Formation Evolution
2009/6/9
Formation and Evolution of Self-Interacting Dark Matter Halos。
Shallow cores in the dark matter halos：self-interaction in action?
dark matter halos self-interaction
2009/6/8
Shallow cores in the dark matter halos：self-interaction in action?
The effect of gasdynamics on the structure of dark matter halos
gasdynamics dark matter halos
2009/6/8
The effect of gasdynamics on the structure of dark matter halos。
The effect of gasdynamics on the structure of dark matter halos
gasdynamics dark matter halos
2009/6/8
The effect of gasdynamics on the structure of dark matter halos。
Dark Matter and the Chemical Evolution of Irregular Galaxies
Dark Matter Irregular Galaxies Chemical Evolution
2009/6/5
Dark Matter and the Chemical Evolution of Irregular Galaxies。
NGC 404, a galaxy without dark matter。
On A Possible Connection Between Chandler Wobble And Dark Matter
Chandler wobble Polar motion Dark matter
2010/7/5
Chandler wobble excitation and damping, one of the open problems in geophysics, is treated as a consequence in part of the interaction between Earth and a hypothetical oblate ellipsoid made of dark ma...
THE CONTRIBUTION OF THE DARK MATTER TO THE ROTATION OF SPIRAL GALAXIES AND ITS MASS DISTRIBUTION
DARK MATTER SPIRAL GALAXIES MASS DISTRIBUTION
2009/3/19
The rotation of a test spiral galaxy with two contributors - the disc
and the corona - is considered. The disc is exponential, whereas the corona is the
dark subsystem. For the latter several varian...
DARK MATTER HALOES：AN ADDITIONAL CRITERION FOR THE CHOICE OF FITTING DENSITY PROFILES
cosmology dark matter
2009/3/5
Simulated dark matter haloes are tted by self-similar, universal
density pro les, where the scaled parameters depend only on a scaled (truncation)
radius, = R=r0, which, in turn, is supposed to b...
A NUMERICAL FIT OF ANALYTICAL TO SIMULATED DENSITY PROFILES IN DARK MATTER HALOES
cosmology theory-dark matter-galaxies clusters galaxies haloes
2009/2/25
A NUMERICAL FIT OF ANALYTICAL TO SIMULATED DENSITY PROFILES IN DARK MATTER HALOES.