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Residual-gas expulsion after cluster formation has recently been shown to leave an imprint in the low-mass present-day stellar mass function (PDMF) which allowed the estimation of birth conditions of ...
We calculated the radial profiles of the azimuthally averaged midplane gas volume density $\rho_g$ for 11 high surface brightness (HSB) spiral galaxies, 7 low surface brightness (LSB) galaxies and 3 S...
Flat central density profiles from scalar field dark matter halos。
The density of the narrow-line region of type 1 Active Galactic Nuclei
A 1.4 GHZ and 14.7 GHZ analysis of density gradients in galactic planetary nebulae。
Determination of the Electron Density in the Orion Nebula with High Spectral Resolution。
Temperature and Density Gradients in the Orion Nebula。
Diagnostic determination of ionization and density in stellar jets from line ratios。
Dusty uch II regions:cloud pressures and density distributions
Density bounded H II regions:ionization of the diffuse interstellar and intergalactic media。
This contribution presents the unique technique of using rock pushing activities to estimate the densities of rocks remotely.
A special case of the generalised Schuster density law for stellar systems with spherical symmetry is discussed; here the exponent in the denominator is equal to i/2 where i is a positive integer. ...
Assuming that the disc of our Galaxy, the Milky Way, obeys the classical exponential law, that it is maximal and the Sun is rather far from the maximum of its circular velocity, one ¯nds that, ...

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