Titlebook: Cosmic Rays in Star-Forming Environments; Proceedings of the S Diego F. Torres,Olaf Reimer Conference proceedings 2013 Springer-Verlag Berl

首創(chuàng)精神

爆米花

Nonthermal Emission from Star-Forming Galaxies,of star-driven nonthermal processes and phenomena in non-AGN star-forming galaxies. We review basic aspects of the related processes and their modeling in starburst galaxies. Since these processes involve both energetic electrons and protons accelerated by SN shocks, their respective radiative yield

航海太平洋

Cosmic Ray Acceleration in W51C Observed with the MAGIC Telescopes, the energy spectrum between 75 GeV and 5.5 TeV, and to fit it with a single power law with an index of 2. 58 ± 0. 07. ± 0. 22.. We look for underlying structures by means of detailed morphological studies that allow us to locate the majority of the emission around the interaction point between W51C

Latency

Cosmic Rays and Molecular Clouds,the dense gas and produce neutral pions which in turn decay into two gamma rays. This makes molecular clouds potential sources of gamma rays, especially if they are located in the vicinity of a powerful accelerator that injects cosmic rays in the interstellar medium. The amplitude and duration in ti

infantile

,Molecular and Atomic Gas in the Young TeV ,-Ray SNRs RX J1713.7–3946 and RX J0852.0–4622; Evidence cess. The interstellar atomic gas is enveloping the molecular clouds and may also be dense enough to affect the .-ray production. In this chapter, some of the basic properties of the interstellar gas both in molecular and atomic forms will be reviewed. Then, it is presented that two young TeV .-ray