Connecting the new H.E.S.S. diffuse emission at the Galactic Center with the Fermi GeV excess: A combination of millisecond pulsars and heavy dark matter?

Suivent les lots d’œufs achetés au niveau des différents points de vente des œufs avec un taux de contamination de 32.22%, puis les lots d’œufs provenant des bâtiments

“The sudden emergence of English as a great literary language at the end of the fourteenth century in the writings of some scholastics such as: Chaucer, Lang land

The gamma- ray and radio pulse shapes and relative lags motivated light curve modeling using standard outer magnetospheric pulsar models commonly employed to describe the light

We explored different spatial models for M33, and the result is that the gamma-ray emission in the direction of M33 is consistent with a point-like source at position (α, δ) =

A successful strategy to solve the problem of light absorption through such molecular layers is found in the application of high surface area films consisting of nanocrystalline

Prospects of indirect detection in the close-by dark matter dominated Sagittarius dwarf galaxy are investigated in MSSM and Kaluza-Klein scenarii.. 2 γ-rays from Dark

compare our best-fit values to this and do not use it to limit the likelihood analysis. Both the OG and TPC model match the observed gamma-ray light curve well, but neither

The second result is that the kinetic energy of rotation of a ball resulting from the compactification of a galactic sized system is enormous, more than thirteen times its own mass