Large bent jets in the inner region of CSSs

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dc.creatorMantovani, F.
dc.creatorJunor, W.
dc.creatorBondi, M.
dc.creatorCotton, W.
dc.creatorFanti, R.
dc.creatorPadrielli, L.
dc.creatorNicolson, G.
dc.creatorSalerno, E.
dc.date1997-12-05
dc.date.accessioned2026-07-07T02:25:30Z
dc.date.available2026-07-07T02:25:30Z
dc.descriptionThe class of Compact Steep-spectrum Sources is dominated by double-lobed objects (70%). The remaining 30% are jet-dominated objects, with the jet brightened either by Doppler boosting or by interaction with the ambient media. We show that there is both observational and statistical evidence in favour of an interaction between jets and dense gas clouds. Such an interaction should happen in the Narrow Line Regions. The images of four CSSs observed by us with VLBI are also presented. These sources do show large bent jets in the first kpc from the nucleus.
dc.description10 pages, plain tex, plus 7 .ps figures, accepted by Astronomy and Astrophysics, Main Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/9712084
dc.identifierhttp://arxiv.org/abs/astro-ph/9712084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11899
dc.subjectAstrophysics
dc.titleLarge bent jets in the inner region of CSSs
dc.typetext

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