Astrophysical sources and acceleration mechanisms
Martina Adamo, Silvia Pietroni, Maurizio Spurio

TL;DR
This paper discusses the role of cosmic rays in multi-messenger astronomy, emphasizing the importance of understanding their sources and acceleration mechanisms through various observational methods.
Contribution
It highlights the significance of cosmic rays in multi-messenger astronomy and underscores the need for further study of their origins and acceleration processes.
Findings
Cosmic rays are crucial in multi-messenger observations.
Understanding acceleration mechanisms is key to cosmic ray research.
Multi-messenger approaches enhance astrophysical insights.
Abstract
Multi-messenger astronomy provides for the observation of the same astronomical event with different kind of telescopes at the same time: optical observations, X-rays, gamma-ray bursts, neutrinos and, most recently, gravitational waves are just few examples of the several points of view from which an astronomical event can be observed and analyzed. Cosmic rays play an important role in multi-messenger astronomy and, for this reason, it is important to deepen the study of their sources and to understand the mechanisms behind their acceleration in astronomical environments.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena
