Radio observations of gamma-ray blazars

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dc.creatorPohl, M.
dc.creatorMuecke, A.
dc.creatorReich, W.
dc.creatorReich, P.
dc.creatorSchlickeiser, R.
dc.creatorUngerechts, H.
dc.date1996-03-22
dc.date.accessioned2026-07-07T02:21:02Z
dc.date.available2026-07-07T02:21:02Z
dc.descriptionStarting in 1991 we have performed a regular monitoring of EGRET sources with the Effelsberg 100-m telescope and the IRAM 30-m at Pico Veleta. In comparison with data on a sample of flat-spectrum quasars which have not been seen by EGRET we search for correlations of any kind in the behaviour of FSRQ's in the radio and gamma-ray regime. While there is no radio-to-gamma-ray luminosity correlation for these sources, it seems that gamma-ray high states coincide with increased activity in the radio regime with a strong tendency that gamma-ray outbursts precede radio outbursts. The gamma-ray spectra seem to harden with increasing flux level.
dc.description6 pages, Proceedings of the "Blazar Variability Workshop", Miami, February 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9603123
dc.identifierhttp://arxiv.org/abs/astro-ph/9603123
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10413
dc.subjectAstrophysics
dc.titleRadio observations of gamma-ray blazars
dc.typetext

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