First high-resolution radio study of the supernova remnant G338.3-0.0 associated with the gamma-ray source HESS J1640-465

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Aims. We perform a multifrequency radio study of the supernova remnant (SNR) G338.3-0.0, in positional coincidence with the TeV source HESS J1640 - 465. We study the morphological and spectral properties of this remnant and its surroundings searching for plausible radio counterparts to the gamma-ray...

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Detalles Bibliográficos
Autores principales: Castelletti, G., Giacani, E., Dubner, G., Joshi, B.C., Rao, A.P., Terrier, R.
Formato: Artículo publishedVersion
Publicado: 2011
Materias:
ISM: individual objects: G338.3-0.0
ISM: individual objects: HESS J1640-465
ISM: supernova remnants
Radio continuum: ISM
Archival data
Australia
Compact arrays
Emission lines
Flux densities
Gamma ray sources
Gamma-ray emission
Giant metrewave radio telescopes
High resolution
Ionized gas
ISM: individual objects
Molecular gas
Molecular materials
Multi frequency
Optical depth
Pulsar wind nebula
Radio flux
Radio frequencies
Radio observation
Spectral indices
Spectral properties
Supernova remnants
Upper limits
Associated gas
Atmospheric optics
Ionization of gases
Optical telescopes
Radio telescopes
Stars
Tellurium compounds
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v536_n_p_Castelletti
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00046361_v536_n_p_Castelletti_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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