Développement d'un simulateur pour le X-ray integral field unit : du signal astrophysique à la performance instrumentale

Fabian (2004), also in our model there are different regimes of vari- ability, essentially depending on the degree of inhomogeneity of the heating rate, h, and on the optical depth

In this paper, we investigate the wavelength and temperature dependence of the magneto- optical properties of a GaMnAs layer with and without capping by dielectric layers using

As there is good evidence that the PhNR to both stimulus on- and the stimulus offset contains such inner retinal information and is affected in glaucoma [ 3 , 4 ] we evaluated

Setting up and maintaining an organizational committee might be a more or less easy thing to do at the local level, due to geographic proximity, but some

As in the presence of a pion condensate young neutron stars cool much i a s t e r ~ q , the philosophy,of this paper (following Maxwellc71) will be to calculate the fas-

The spectra of pulsating X-ray sources the dynamic behavior of the Crab and Vela can provide information about the strength pulsars following sudden spinup,-/ Their of the

My work has been mostly organized into two steps: the first part concerned the study of the dynamics of accretion disks around neutron stars which allowed me to familiarize myself

We carry out a set of simulations, considering a fixed black hole spin (0.5), with reflection computed in a fixed lamp-post configuration, blueshifting the third absorber component