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dc.contributor.authorMontenegro Monte, F.M.
dc.contributor.authorMack, K.-H.
dc.contributor.authorBenn, C.R.
dc.contributor.authorCarballo Fidalgo, Ruth 
dc.contributor.authorDallacasa, D.
dc.contributor.authorGonzález Serrano, José Ignacio 
dc.contributor.authorHolt, J.
dc.contributor.authorJimenez Lujan, Florencia
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-01-20T14:47:43Z
dc.date.available2023-01-20T14:47:43Z
dc.date.issued2008
dc.identifier.issn1824-8039
dc.identifier.urihttps://hdl.handle.net/10902/27339
dc.description.abstractBroad Absorption Line Quasars (BAL QSOs) have been found to be associated with extremely compact radio sources. These reduced dimensions can be either due to projection effects or these objects might actually be intrinsically small. Exploring these two hypotheses is important to understand the nature and origin of the BAL phenomenon because orientation effects are an important discriminant between the different models proposed to explain this phenomenon. In this work we present VLBA observations of 5 BAL QSOs and discuss their pc-scale morphologyes_ES
dc.format.extent6 p.es_ES
dc.language.isoenges_ES
dc.publisherSissa Medialabes_ES
dc.rights© Los autores.es_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/*
dc.sourcePoS - Proceedings of science, 2008, 72, 019es_ES
dc.titleVLBA imaging of radio-loud BAL QSOses_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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