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Abstract:

The giant molecular clouds (MCs) found in the Milky Way and similar galaxies play a crucial role in the evolution of these systems. The supernova explosions that mark the death of massive stars in these regions often lead to interactions between the supernova remnants (SNRs) and the clouds. These interactions have a profound effect on our understanding of SNRs. Shocks in SNRs should be capable of accelerating particles to cosmic ray (CR) energies with efficiencies high enough to power Galactic CRs. X-ray and γ-ray studies have established the presence of relativistic electrons and protons in some SNRs and provided strong evidence for diffusive shock acceleration as the primary acceleration mechanism, including strongly amplified magnetic fields, temperature and ionization effects on the shock-heated plasmas, and modifications to the dynamical evolution of some systems. Because protons dominate the overall energetics of the CRs, it is crucial to understand this hadronic component even though electrons are much more efficient radiators and it can be difficult to identify the hadronic component. However, near MCs the densities are sufficiently high to allow the γ-ray emission to be dominated by protons. Thus, these interaction sites provide some of our best opportunities to constrain the overall energetics of these particle accelerators. Here we summarize some key properties of interactions between SNRs and MCs, with an emphasis on recent X-ray and γ-ray studies that are providing important constraints on our understanding of cosmic rays in our Galaxy. © 2014, Springer Science+Business Media Dordrecht.

Registro:

Documento: Artículo
Título:Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures
Autor:Slane, P.; Bykov, A.; Ellison, D.C.; Dubner, G.; Castro, D.
Filiación:Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, United States
Ioffe Institute for Physics and Technology, St. Petersburg, 194021, Russian Federation
St. Petersburg State Polytechnical University, St. Petersburg, Russian Federation
Physics Department, North Carolina State University, Box 8202, Raleigh, NC 27695, United States
Instituto de Astronomía y Física del Espacio (IAFE), UBA-CONICET, CC 67, Suc. 28, Buenos Aires, 1428, Argentina
MIT-Kavli Center for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139, United States
Palabras clave:Gamma-rays; Molecular clouds; Supernova remnants; X-rays; Astronomy; Clouds; Cosmic rays; Galaxies; Supernovae; X rays; Acceleration mechanisms; Diffusive shock accelerations; Dynamical evolution; Giant molecular clouds; Molecular clouds; Relativistic electron; Supernova explosion; Supernova remnants; Gamma rays
Año:2015
Volumen:188
Número:1-4
Página de inicio:187
Página de fin:210
DOI: http://dx.doi.org/10.1007/s11214-014-0062-6
Título revista:Space Science Reviews
Título revista abreviado:Space Sci Rev
ISSN:00386308
CODEN:SPSRA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00386308_v188_n1-4_p187_Slane

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Citas:

---------- APA ----------
Slane, P., Bykov, A., Ellison, D.C., Dubner, G. & Castro, D. (2015) . Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures. Space Science Reviews, 188(1-4), 187-210.
http://dx.doi.org/10.1007/s11214-014-0062-6
---------- CHICAGO ----------
Slane, P., Bykov, A., Ellison, D.C., Dubner, G., Castro, D. "Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures" . Space Science Reviews 188, no. 1-4 (2015) : 187-210.
http://dx.doi.org/10.1007/s11214-014-0062-6
---------- MLA ----------
Slane, P., Bykov, A., Ellison, D.C., Dubner, G., Castro, D. "Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures" . Space Science Reviews, vol. 188, no. 1-4, 2015, pp. 187-210.
http://dx.doi.org/10.1007/s11214-014-0062-6
---------- VANCOUVER ----------
Slane, P., Bykov, A., Ellison, D.C., Dubner, G., Castro, D. Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures. Space Sci Rev. 2015;188(1-4):187-210.
http://dx.doi.org/10.1007/s11214-014-0062-6