Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

Interstellar and circumstellar matter.-- et al.

Detalles Bibliográficos
Autores: Barreiro, R. Belén, Curto, Andrés, Diego, José María, González-Nuevo, J., Herranz, Diego, López-Caniego, M., Macías-Pérez, J. F., Martínez-González, Enrique, Toffolatti, Luigi, Vielva, Patricio, Reach, W. T., Planck Collaboration
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2016
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/140623
Acceso en línea:http://hdl.handle.net/10261/140623
Access Level:acceso abierto
Palabra clave:ISM: supernova remnants
Cosmic rays
Radio continuum: ISM
id ES_641fcea4c8e3366297a349df2db9a596
oai_identifier_str oai:digital.csic.es:10261/140623
network_acronym_str ES
network_name_str España
repository_id_str
spelling Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnantsBarreiro, R. BelénCurto, AndrésDiego, José MaríaGonzález-Nuevo, J.Herranz, DiegoLópez-Caniego, M.Macías-Pérez, J. F.Martínez-González, EnriqueToffolatti, LuigiVielva, PatricioReach, W. T.Planck CollaborationISM: supernova remnantsCosmic raysRadio continuum: ISMInterstellar and circumstellar matter.-- et al.The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck frequencies. The radio-through-microwave spectral energy distributions were compiled to determine the mechanism for microwave emission. In only one case, IC 443, is there high-frequency emission clearly from dust associated with the supernova remnant. In all cases, the low-frequency emission is from synchrotron radiation. As predicted for a population of relativistic particles with energy distribution that extends continuously to high energies, a single power law is evident for many sources, including the Crab and PKS 1209-51/52. A decrease in flux density relative to the extrapolation of radio emission is evident in several sources. Their spectral energy distributions can be approximated as broken power laws, Sν ∝ ν−α, with the spectral index, α, increasing by 0.5–1 above a break frequency in the range 10–60 GHz. The break could be due to synchrotron losses.The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU).Peer ReviewedEDP SciencesCenter for Science (Finland)Academy of FinlandScience and Technology Facilities Council (UK)NASAIstituto Nazionale di AstrofisicaCentre National de la Recherche Scientifique (France)European Space AgencyJunta de AndalucíaConsejo Superior de Investigaciones Científicas (España)Ministerio de Economía y Competitividad (España)European CommissionEuropean Research CouncilAgenzia Spaziale ItalianaDepartment of Energy (US)UK Space AgencyFundação para a Ciência e a Tecnologia (Portugal)German Centre for Air and Space TravelMax Planck SocietyScience Foundation IrelandDTU Space (Denmark)Swiss Space OfficeConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2016201620162016info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/140623reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1051/0004-6361/201425022Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1406232026-05-22T06:33:51Z
dc.title.none.fl_str_mv Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
title Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
spellingShingle Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
Barreiro, R. Belén
ISM: supernova remnants
Cosmic rays
Radio continuum: ISM
title_short Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
title_full Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
title_fullStr Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
title_full_unstemmed Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
title_sort Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants
dc.creator.none.fl_str_mv Barreiro, R. Belén
Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Macías-Pérez, J. F.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Reach, W. T.
Planck Collaboration
author Barreiro, R. Belén
author_facet Barreiro, R. Belén
Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Macías-Pérez, J. F.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Reach, W. T.
Planck Collaboration
author_role author
author2 Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Macías-Pérez, J. F.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Reach, W. T.
Planck Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Center for Science (Finland)
Academy of Finland
Science and Technology Facilities Council (UK)
NASA
Istituto Nazionale di Astrofisica
Centre National de la Recherche Scientifique (France)
European Space Agency
Junta de Andalucía
Consejo Superior de Investigaciones Científicas (España)
Ministerio de Economía y Competitividad (España)
European Commission
European Research Council
Agenzia Spaziale Italiana
Department of Energy (US)
UK Space Agency
Fundação para a Ciência e a Tecnologia (Portugal)
German Centre for Air and Space Travel
Max Planck Society
Science Foundation Ireland
DTU Space (Denmark)
Swiss Space Office
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv ISM: supernova remnants
Cosmic rays
Radio continuum: ISM
topic ISM: supernova remnants
Cosmic rays
Radio continuum: ISM
description Interstellar and circumstellar matter.-- et al.
publishDate 2016
dc.date.none.fl_str_mv 2016
2016
2016
2016
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/140623
url http://hdl.handle.net/10261/140623
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv http://dx.doi.org/10.1051/0004-6361/201425022
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869409622740172800
score 15,812429

Similares en LA Referencia