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We construct a gas temperature map for the IRDC, with the highest angular resolution available to date for this source and, wherever deemed signi ficant, for separate

Moreover, we can trace the particles’ propagation outside the neutron stars’ magnetospheres through their synchrotron emission, responsible for X-ray extended features, and their

Fitting the extracted spectrum with a sample of spectra of low mass objects, we were able to classify HR 2562 B as an early T (T2-T3) spectral type, although the H broad-band

(Colour online) Reflectance spectrum of the asteroid (311999) 2007 NS2 (black dotted line) compared with average spectra for A (red), S.. (green) and S a (purple)

We further demonstrate that our results are not showing redshift trends by constraining the mass and observable bias parameters for each tested scaling relation in two

• definition of a possible strategy to be adopted for Demand Planning and Supply Planning, according to customer requirements, for future developments;

In questa tesi abbiamo applicato per la prima volta il metodo RG alla gravit`a massiva nella teoria non Fierz-Pauli, abbiamo studiato la teoria dal settore IR, dove presenta

Using time- resolved high-resolution X-ray spectroscopy of a stellar flare on the active star HR 9024 observed with Chandra/HETGS, we distinctly detected Doppler shifts in S xvi,