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

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發(fā)表于 2025-3-21 17:06:50 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Cosmic Rays in Star-Forming Environments
副標(biāo)題Proceedings of the S
編輯Diego F. Torres,Olaf Reimer
視頻videohttp://file.papertrans.cn/239/238898/238898.mp4
概述Presents state-of-the art results on cosmic-ray research.Includes supplementary material:
叢書(shū)名稱Astrophysics and Space Science Proceedings
圖書(shū)封面Titlebook: Cosmic Rays in Star-Forming Environments; Proceedings of the S Diego F. Torres,Olaf Reimer Conference proceedings 2013 Springer-Verlag Berl
描述.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..
出版日期Conference proceedings 2013
關(guān)鍵詞Astroparticle acceleration; Cosmic Ray Workshop; Cosmic accelerators; Cosmic gamma-ray emitters; Cosmic
版次1
doihttps://doi.org/10.1007/978-3-642-35410-6
isbn_softcover978-3-642-43947-6
isbn_ebook978-3-642-35410-6Series ISSN 1570-6591 Series E-ISSN 1570-6605
issn_series 1570-6591
copyrightSpringer-Verlag Berlin Heidelberg 2013
The information of publication is updating

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Martina Zeleňáková,Abdelazim M. Negmexternal galaxies. We will review the methodologies employed to determine the cosmic ray ionization rates in the ISM, how cosmic rays rates can influence the determination of the mass of a galaxy and, finally, how cosmic rays affect star formation and its rate.
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D. Káposztásová,Z. Vranayová,P. Purczl stellar radiation propagating through the dusty ISM of galaxies. It is in such CR-dominated regions (CRDRs) rather than Photon-dominated regions (PDRs) of H. clouds where the star formation initial conditions are set, making CRs the ultimate star-formation feedback factor in galaxies, able to oper
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How to Reach a Point of No Return,o determine the cosmic-ray ionisation rate (especially the cosmic-ray spectrum at . < 1 GeV and the ionisation cross sections), and calculate the ionisation rate as a function of the column density of molecular hydrogen. Available data support the existence of a low-energy component (below ～ 100 MeV
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Space as the Next Theater of War,. These processes drive the chemical pathways of formation of gas phase molecules which later can be adsorbed onto the surface of grains. We improve on previously existing chemical models by treating the interaction of cosmic rays with the gas/grain environment in a way that is consistent with the l
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