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The Ks band differential star count of the Two Micron All Sky Survey (2MASS) is used to derive the global structure parameters of the smooth components of the Milky Way. To avoid complication introduc...
We analyze the dependence of galaxy structure (size and Sersic index) and mode of star formation (\Sigma_SFR and SFR_IR/SFR_UV) on the position of galaxies in the SFR versus Mass diagram. Our sample c...
Microlensing is now a very popular observational astronomical technique. The investigations accessible through this effect range from the dark matter problem to the search for extra-solar planets. In ...
Microlensing probes the AGN structure of the lensed quasar J1131-1231。
Disk structure and evolution around the neutron star in Be/x-ray binaries。
The implications of disc instabilities on cataclysmic Variable structure and evolution。
Clouds and Instabilities in Supernova Remnant Structure:Interstellar Turbulence and Rippled Shocks。
Structure and Behavior of Ionized Stellar Winds。
The Winds of O-Type Stars:Ionization Structure and Revised Stellar Parameters from Far-UV Spectra。
The structure of halos in Self-Interacting Cold Dark Matter models。

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