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Abstract:

The explosion of a supernova releases almost instantaneously about 10$$^{51}$$51 ergs of mechanic energy, changing irreversibly the physical and chemical properties of large regions in the galaxies. The stellar ejecta, the nebula resulting from the powerful shock waves, and sometimes a compact stellar remnant, constitute a supernova remnant (SNR). They can radiate their energy across the whole electromagnetic spectrum, but the great majority are radio sources. Almost 70 years after the first detection of radio emission coming from an SNR, great progress has been achieved in the comprehension of their physical characteristics and evolution. We review the present knowledge of different aspects of radio remnants, focusing on sources of the Milky Way and the Magellanic Clouds, where the SNRs can be spatially resolved. We present a brief overview of theoretical background, analyze morphology and polarization properties, and review and critically discuss different methods applied to determine the radio spectrum and distances. The consequences of the interaction between the SNR shocks and the surrounding medium are examined, including the question of whether SNRs can trigger the formation of new stars. Cases of multispectral comparison are presented. A section is devoted to reviewing recent results of radio SNRs in the Magellanic Clouds, with particular emphasis on the radio properties of SN 1987A, an ideal laboratory to investigate dynamical evolution of an SNR in near real time. The review concludes with a summary of issues on radio SNRs that deserve further study, and analysis of the prospects for future research with the latest-generation radio telescopes. © 2015, Springer-Verlag Berlin Heidelberg.

Registro:

Documento: Artículo
Título:Radio emission from supernova remnants
Autor:Dubner, G.; Giacani, E.
Filiación:Instituto de Astronomía y Física del Espacio (IAFE), CONICET-UBA, Casilla de Correo 67, Suc. 28, Buenos Aires, 1428, Argentina
Palabras clave:ISM: cosmic rays; ISM: supernova remnants; Radiation mechanisms: non-thermal; Radio continuum: ISM; Balloons; Cosmology; Galaxies; Radio astronomy; Shock waves; Stars; Electromagnetic spectra; ISM: cosmic rays; ISM: supernova remnants; Physical and chemical properties; Physical characteristics; Polarization properties; Radiation mechanisms: non thermal; Radio continuum: ISM; Supernovae
Año:2015
Volumen:23
Número:1
DOI: http://dx.doi.org/10.1007/s00159-015-0083-5
Título revista:Astronomy and Astrophysics Review
Título revista abreviado:Astronom Astrophys Rev
ISSN:09354956
CODEN:AASRE
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09354956_v23_n1_p_Dubner

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Citas:

---------- APA ----------
Dubner, G. & Giacani, E. (2015) . Radio emission from supernova remnants. Astronomy and Astrophysics Review, 23(1).
http://dx.doi.org/10.1007/s00159-015-0083-5
---------- CHICAGO ----------
Dubner, G., Giacani, E. "Radio emission from supernova remnants" . Astronomy and Astrophysics Review 23, no. 1 (2015).
http://dx.doi.org/10.1007/s00159-015-0083-5
---------- MLA ----------
Dubner, G., Giacani, E. "Radio emission from supernova remnants" . Astronomy and Astrophysics Review, vol. 23, no. 1, 2015.
http://dx.doi.org/10.1007/s00159-015-0083-5
---------- VANCOUVER ----------
Dubner, G., Giacani, E. Radio emission from supernova remnants. Astronom Astrophys Rev. 2015;23(1).
http://dx.doi.org/10.1007/s00159-015-0083-5