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dc.creatorGabanyi, K. E.-
dc.creatorDubner, Gloria Mabel-
dc.creatorGiacani, Elsa Beatriz-
dc.creatorParagi, Z.-
dc.creatorFrey, S.-
dc.creatorPidopryhora, Y.-
dc.date2015-06-09T17:47:45Z-
dc.date2015-06-09T17:47:45Z-
dc.date2013-01-01-
dc.date2016-03-30 10:35:44.97925-03-
dc.date.accessioned2019-04-29T15:44:01Z-
dc.date.available2019-04-29T15:44:01Z-
dc.date.issued2015-06-09T17:47:45Z-
dc.date.issued2015-06-09T17:47:45Z-
dc.date.issued2013-01-01-
dc.date.issued2016-03-30 10:35:44.97925-03-
dc.identifierGabanyi, K. E.; Dubner, Gloria Mabel; Giacani, Elsa Beatriz; Paragi, Z.; Frey, S.; et al.; Very Long Baseline Interferometry Search for The Radio Counterpart Of Hess J1943+213; Iop Publishing Ltd; Astrophysical Journal; 762; 1-1-2013; 63-70-
dc.identifier0004-637X-
dc.identifierhttp://hdl.handle.net/11336/648-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/300609-
dc.descriptionHESS J1943+213, a TeV point source close to the Galactic plane recently discovered by the H.E.S.S. Collaboration, was proposed to be an extreme BL Lacertae object, though a pulsar wind nebula (PWN) nature could not be completely discarded. To investigate its nature, we performed high-resolution radio observations with the European Very Long Baseline Interferometry Network (EVN) and reanalyzed archival continuum and H I data. The EVN observations revealed a compact radio counterpart of the TeV source. The low brightness temperature and the resolved nature of the radio source are indications against the beamed BL Lacertae hypothesis. The radio/X-ray source appears immersed in a ~1´ elliptical feature, suggesting a possible galactic origin (PWN nature) for the HESS source. We found that HESS J1943+213 is located in the interior of a ~1° diameter H I feature and explored the possibility of them being physically related.-
dc.descriptionFil: Gabanyi, K. E.. Konkoly Observatory. Research Centre for Astronomy and Earth Sciences of the Hungarian Academy of Sciences; Hungría;-
dc.descriptionFil: Dubner, Gloria Mabel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina-
dc.descriptionFil: Giacani, Elsa Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio(i); Argentina. FADU. Universidad Nacional de Buenos Aires; Argentina-
dc.descriptionFil: Paragi, Z.. Joint Institute for VLBI in Europe; Holanda;-
dc.descriptionFil: Frey, S.. FÖMI Satellite Geodetic Observator; Hungría;-
dc.descriptionFil: Pidopryhora, Y.. Joint Institute for VLBI in Europe; Holanda;-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIop Publishing Ltd-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/0004-637X/762/1/63-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/0004-637X/762/1/63-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1110.5039v4-
dc.rightsinfo:eu-repo/semantics/restrictedAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.subjectISM:supernova remnants-
dc.subjectradio continuum:general, radio lines-
dc.subjectISM,technics:interferometric-
dc.subjectX-rays: individuals: CXOU J194356.2+211823-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleVery Long Baseline Interferometry Search for The Radio Counterpart Of Hess J1943+213-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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