E-MERLIN observations of the puzzling TeV source HESS J1943+213

HESS J1943+213 is a TeV source close to the Galactic plane proposed to be a BL Lac object. Our high resolution EVN observation failed to recover two thirds of the source flux density detected simultaneously by the WSRT. Our recent e-MERLIN observations in L and C bands show only a point source with...

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Autores principales: Gabányi, K.É., Dubner, G., Giacani, E., Frey, S., Paragi, Z.
Formato: CONF
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Gabanyi
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spelling todo:paper_18248039_v_n_p_Gabanyi2023-10-03T16:33:09Z E-MERLIN observations of the puzzling TeV source HESS J1943+213 Gabányi, K.É. Dubner, G. Giacani, E. Frey, S. Paragi, Z. Extragalactic sources Flux densities Galactic plane High resolution Line of Sight Point sources Scale sizes Source flux Tellurium compounds HESS J1943+213 is a TeV source close to the Galactic plane proposed to be a BL Lac object. Our high resolution EVN observation failed to recover two thirds of the source flux density detected simultaneously by the WSRT. Our recent e-MERLIN observations in L and C bands show only a point source with flux density comparable to the EVN detection. Thus the structure responsible for the missing flux density has to be larger than 2". It may be related to the presumed extragalactic source (thus would have a kpc-scale size), or to the Galactic foreground material close to the line of sight to the source. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Gabanyi
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Extragalactic sources
Flux densities
Galactic plane
High resolution
Line of Sight
Point sources
Scale sizes
Source flux
Tellurium compounds
spellingShingle Extragalactic sources
Flux densities
Galactic plane
High resolution
Line of Sight
Point sources
Scale sizes
Source flux
Tellurium compounds
Gabányi, K.É.
Dubner, G.
Giacani, E.
Frey, S.
Paragi, Z.
E-MERLIN observations of the puzzling TeV source HESS J1943+213
topic_facet Extragalactic sources
Flux densities
Galactic plane
High resolution
Line of Sight
Point sources
Scale sizes
Source flux
Tellurium compounds
description HESS J1943+213 is a TeV source close to the Galactic plane proposed to be a BL Lac object. Our high resolution EVN observation failed to recover two thirds of the source flux density detected simultaneously by the WSRT. Our recent e-MERLIN observations in L and C bands show only a point source with flux density comparable to the EVN detection. Thus the structure responsible for the missing flux density has to be larger than 2". It may be related to the presumed extragalactic source (thus would have a kpc-scale size), or to the Galactic foreground material close to the line of sight to the source. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
format CONF
author Gabányi, K.É.
Dubner, G.
Giacani, E.
Frey, S.
Paragi, Z.
author_facet Gabányi, K.É.
Dubner, G.
Giacani, E.
Frey, S.
Paragi, Z.
author_sort Gabányi, K.É.
title E-MERLIN observations of the puzzling TeV source HESS J1943+213
title_short E-MERLIN observations of the puzzling TeV source HESS J1943+213
title_full E-MERLIN observations of the puzzling TeV source HESS J1943+213
title_fullStr E-MERLIN observations of the puzzling TeV source HESS J1943+213
title_full_unstemmed E-MERLIN observations of the puzzling TeV source HESS J1943+213
title_sort e-merlin observations of the puzzling tev source hess j1943+213
url http://hdl.handle.net/20.500.12110/paper_18248039_v_n_p_Gabanyi
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AT giacanie emerlinobservationsofthepuzzlingtevsourcehessj1943213
AT freys emerlinobservationsofthepuzzlingtevsourcehessj1943213
AT paragiz emerlinobservationsofthepuzzlingtevsourcehessj1943213
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