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dc.contributor.author
Reynoso, Estela Marta
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dc.contributor.author
Walsh, A. J.
dc.date.available
2017-06-06T18:35:33Z
dc.date.issued
2015-08
dc.identifier.citation
Reynoso, Estela Marta; Walsh, A. J.; Radio spectral characteristics of the supernova remnant Puppis A and nearby sources; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 451; 3; 8-2015; 3044-3054
dc.identifier.issn
0035-8711
dc.identifier.uri
http://hdl.handle.net/11336/17585
dc.description.abstract
This paper presents a new study of the spectral index distribution of the supernova remnant (SNR) Puppis A. The nature of field compact sources is also investigated according to the measured spectral indices. This work is based on new observations of Puppis A and its surroundings performed with the Australia Telescope Compact Array in two configurations using the Compact Array Broad-band Backend centred at 1.75 GHz. We find that the global spectral index of Puppis A is α = −0.563 ± 0.013. Local variations have been detected, however this global index represents well the bulk of the SNR. At the SE, we found a pattern of parallel strips with a flat spectrum compatible with small-scale filaments, although not correlated in detail. The easternmost filament agrees with the idea that the SNR shock front is interacting with an external cloud. There is no evidence of the previously suggested correlation between emissivity and spectral index. A number of compact features are proposed to be evolved clumps of ejecta based on their spectral indices, although dynamic measurements are needed to confirm this hypothesis.We estimate precise spectral indices for the five previously known field sources, two of which are found to be double (one of them, probably triple), and catalogue 40 new sources. In the light of these new determinations, the extragalactic nature previously accepted for some compact sources is now in doubt.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Oxford University Press
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dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Radiation Mechanisms: Non-Thermal
dc.subject
Techniques: Interferometric
dc.subject
Ism: Individual Objects: Puppis A
dc.subject
Ism: Supernova Remnants
dc.subject
Radio Continuum: Ism
dc.subject.classification
Astronomía
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dc.subject.classification
Ciencias Físicas
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dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
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dc.title
Radio spectral characteristics of the supernova remnant Puppis A and nearby sources
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-06-06T14:48:20Z
dc.journal.volume
451
dc.journal.number
3
dc.journal.pagination
3044-3054
dc.journal.pais
Reino Unido
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dc.journal.ciudad
Londres
dc.description.fil
Fil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
dc.description.fil
Fil: Walsh, A. J.. Curtin University; Australia
dc.journal.title
Monthly Notices Of The Royal Astronomical Society
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dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/451/3/3044/1193040/Radio-spectral-characteristics-of-the-supernova?redirectedFrom=fulltext
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stv1147
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1506.03801
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