Spectro-Morphology of Galaxies.

Elle s'y était risqué et petit à petit, elle s'était prise au jeu, menant une double vie et deux fois par semaine, elle se grimait d'une perruque brune,

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All, they find, using different forms for the disk and often Einstein equations, similar results: the Bessel’s functions, similar mass, …, with no need of a

By means of a high-resolution N-body simulation, we have stud- ied the large-scale variations in stellar metallicity in the disk of a spiral galaxy consisting of cospatial

Dynamical masses of early-type galaxies: a comparison to lensing results and implications for the stellar initial mass function and the distribution of dark matter.. Dark halo

We have included only data from the ALHAMBRA (Advanced Large Homogeneous Area Medium Band Redshift Astronomical) survey and the GALEX (Galaxy Evolution Explorer) mission to

Because all scales contribute to a varying degree to the classification process, the method is relatively robust to shadow effects, missing data and irregular point density (e.g. 9b

To test if our material could provide sufficient drug elution in PJI situation while maintaining the necessary mechanical strength for use as prosthetic joints, we compared