dc.creatorParedes, J. M.
dc.creatorMartí, J.
dc.creatorIshwara Chandra, C. H.
dc.creatorTorres, Diego F.
dc.creatorRomero, Gustavo Esteban
dc.creatorCombi, Jorge Ariel
dc.creatorBosch Ramon, V.
dc.creatorMuñoz Arjonilla, A. J.
dc.creatorSánchez Sutil, J. R.
dc.date2008
dc.date2019-10-28T14:27:03Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84182
dc.identifierissn:0004-6361
dc.descriptionContext. A considerable fraction of the -ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been properly identified are either pulsars or variable sources at both radio and gamma-ray wavelengths. Most of the variable sources are strong radio blazars. However, some low galactic-latitude EGRET sources, with highly variable -ray emission, lack any evident counterpart according to the radio data available until now. Aims. The primary goal of this paper is to identify and characterise the potential radio counterparts of four highly variable -ray sources in the galactic plane through mapping the radio surroundings of the EGRET confidence contours and determining the variable radio sources in the field whenever possible. Methods. We have carried out a radio exploration of the fields of the selected EGRET sources using the Giant Metrewave Radio Telescope (GMRT) interferometer at 21 cm wavelength, with pointings being separated by months. Results. We detected a total of 151 radio sources. Among them, we identified a few radio sources whose flux density has apparently changed on timescales of months. Despite the limitations of our search, their possible variability makes these objects a top-priority target for multiwavelength studies of the potential counterparts of highly variable, unidentified gamma-ray sources.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto Argentino de Radioastronomía
dc.formatapplication/pdf
dc.format247-253
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectGamma rays: observations
dc.subjectRadio continuum: stars
dc.subjectX-rays: binaries
dc.titleRadio detections towards unidentified variable EGRET sources
dc.typeArticulo
dc.typeArticulo


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