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Cosmic Ray Acceleration Inside Molecular Clouds

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Multiwavelength Approach to Unidentified Gamma-Ray Sources

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Abstract

Acceleration of charged particles by neutral gas turbulence in giant molecular clouds is considered. The gamma-ray emission from these clouds is estimated. It is shown that molecular clouds can be the counterparts of some of unidentified sources.

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Author information

Authors and Affiliations

  1. P.N. Lebedev Physical Institute, Leninskii pr. 53, Moscow, Russia

    V.A. Dogiel, A.V. Gurevich, Ya.N. Istomin & K.P. Zybin

Authors
  1. V.A. Dogiel
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  2. A.V. Gurevich
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  3. Ya.N. Istomin
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  4. K.P. Zybin
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Editor information

Editors and Affiliations

  1. University of Hong Kong, China

    K.S. Cheng

  2. Instituto Argentino de Radioastronomia, Buenos Aires, Argentina

    G.E. Romero

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© 2005 Springer

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Dogiel, V., Gurevich, A., Istomin, Y., Zybin, K. (2005). Cosmic Ray Acceleration Inside Molecular Clouds. In: Cheng, K., Romero, G. (eds) Multiwavelength Approach to Unidentified Gamma-Ray Sources. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3881-X_20

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  • DOI: https://doi.org/10.1007/1-4020-3881-X_20

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  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-1-4020-3214-1

  • Online ISBN: 978-1-4020-3881-5

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

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