Search for very-high-energy γ-ray emission from Galactic globular clusters with H.E.S.S.

exposure of individual observation periods (as represented on Fig. SN 2016adj was observed every night from day 3 till day 10 after the discovery date, and the average time

We found several 3FGL sources that have spectra consistent with PBHs, but none of these sources exhibit proper motion, which would be the smoking-gun signature of a PBH in the

Songez à nos conversations longues ou brèves lorsqu’il leur arrive de quitter leur logement et on conviendra que l’immensité de mes locaux leur permet de le

The X-ray analysis of compound 3, as will be shown below, clearly indicates that compound 3 exists as the keto form 3b in the solid state and the nitrogen atom from the piperidine

In addition, those models would also help to prevent ru- mor spreading [101 - 102] and trend detection [103] ; (v) the multi-layered network [104] consists of user social

We analyse the intensity of nuclear de-excitation lines in the direction of the Galactic center produced by subrelativistic protons, which are generated by star capture by the

The black solid line represents the total emission; the red line represents the synchrotron emission by leptons; the green line the SSC component; the pink line the EIC

ةرمثم ةكارإش ءانبو ،عادبلا جمارب زيزعتو ايلعلا تاساردلاو ."عمتجملا عم ةيعإقاو ةلاسرل ةيرئازجلا انتاعماج رقتفت ديدشلا فسلل ريغو بّيغم ةيؤرلا