277 citations · 3.5k across the 94 of their papers we have counts for
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Mass and wind luminosity of young Galactic open clusters in Gaia DR2
Silvia Celli, Andreas Specovius, Stefano Menchiari +2
Context. Star clusters constitute a significant part of the stellar population in our Galaxy. The feedback processes they exert on the interstellar medium impact multiple physical…
Contribution to Galactic cosmic rays from young stellar clusters
G. Morlino, S. Menchiari, E. Amato +1
The origin of Galactic cosmic rays (CR) is still a matter of debate. Diffusive shock acceleration (DSA) applied to supernova remnant (SNR) shocks provides the most reliable explana…
Prospects for -ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array
The Cherenkov Telescope Array Consortium, :, K. Abe +564
Galaxy clusters are expected to be dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly…
Different spectra of cosmic ray H, He and heavier nuclei escaping compact star clusters
Pasquale Blasi, Giovanni Morlino
Cosmic ray acceleration at the termination shock of compact star clusters has recently received much attention, mainly because of the detection of gamma ray emission from some of s…
High energy cosmic rays and gamma rays from star clusters: the case of Cygnus OB2
Pasquale Blasi, Giovanni Morlino
We investigate the acceleration of cosmic rays at the termination shock that results from the interaction of the collective wind of star clusters with the surrounding interstellar…
Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
The Cherenkov Telescope Array Consortium, F. Acero, A. Acharyya +356
The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadr…