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dc.date.accessioned 2021-09-02T14:14:24Z
dc.date.available 2021-09-02T14:14:24Z
dc.date.issued 2005
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/124034
dc.description.abstract We present preliminary results of a campaign undertaken with different radio interferometers to observe a sample of the most variable unidentified EGRET sources. We expect to detect which of the possible counterparts of the γ-ray sources (any of the radio emitters in the field) varies in time with similar timescales as the γ-ray variation. If the γ-rays are produced in a jet-like source, as we have modelled theoretically, synchrotron emission is also expected at radio wavelengths. Such radio emission should appear variable in time and correlated with the γ-ray variability. en
dc.format.extent 223-233 es
dc.language es es
dc.subject γ-ray sources es
dc.subject radio sources es
dc.subject microquasars es
dc.subject microblazars es
dc.title Identifying variable γ-ray sources through radio observations en
dc.type Articulo es
sedici.identifier.other doi:10.1007/1-4020-3881-x_22 es
sedici.identifier.issn 0004-640X es
sedici.identifier.issn 1572-946X es
sedici.creator.person Paredes, Josep M. es
sedici.creator.person Martí, Josep es
sedici.creator.person Torres, Diego F. es
sedici.creator.person Romero, Gustavo Esteban es
sedici.creator.person Combi, Jorge Ariel es
sedici.creator.person Bosch Ramon, Valentí es
sedici.creator.person Garcia Sanchez, J. es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astrophysics and Space Science es
sedici.relation.journalVolumeAndIssue vol. 297, no. 1 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)