Cosmic Rays in Star Forming Environments

These are the proceedings of the Sant Cugat Forum 2nd Workshop on Cosmic-ray Induced Phenomenology in Stellar Environments, held April 16-19, 2012.

Cosmic Rays in Star Forming Environments

These are the proceedings of the Sant Cugat Forum 2nd Workshop on Cosmic-ray Induced Phenomenology in Stellar Environments, held April 16-19, 2012. The aim of this Workshop was to address the current knowledge and challenges of high-energy emission from stellar environments at all scales and provide a comprehensive review of the state of the field from the observational to the theoretical perspectives. In the meeting, the prospects for possible observations with planned instruments across the multi-wavelength spectrum were analyzed and also how they impact on our understanding of these systems.

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Cosmic Rays in Star-Forming Environments
Language: en
Pages: 446
Authors: Diego F. Torres, Olaf Reimer
Categories: Science
Type: BOOK - Published: 2013-04-19 - Publisher: Springer Science & Business Media

These are the proceedings of the Sant Cugat Forum 2nd Workshop on Cosmic-ray Induced Phenomenology in Stellar Environments, held April 16-19, 2012. The aim of this Workshop was to address the current knowledge and challenges of high-energy emission from stellar environments at all scales and provide a comprehensive review of
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Language: en
Pages: 280
Authors: Erik Bertram
Categories: Science
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The aim of this book is to study the role of interstellar turbulence in the process of star formation. We demonstrate that supersonic turbulent motions significantly affect various properties of the interstellar medium. Therefore, we run numerical simulations of molecular clouds in different environments. In particular, we study typical clouds
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Language: en
Pages:
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Type: BOOK - Published: 2021-04-29 - Publisher: Cambridge University Press

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Language: en
Pages: 252
Authors: Silvia Celli
Categories: Science
Type: BOOK - Published: 2019-12-17 - Publisher: Springer Nature

This book addresses three “hot” topics concerning the general problem of the origin of Galactic cosmic rays, namely (1) the acceleration, propagation, and radiation of particles in supernova remnants; (2) very high energy neutrinos from the Galactic Center; and (3) the potential held by the next-generation gamma-ray and neutrino detectors