A high-resolution multi-wavelength study of the jet in 3C 273

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dc.creatorJester, S.
dc.creatorRoeser, H. -J.
dc.creatorMeisenheimer, K.
dc.creatorPerley, R.
dc.creatorGarrington, S.
dc.date2000-11-22
dc.date.accessioned2026-07-07T01:56:39Z
dc.date.available2026-07-07T01:56:39Z
dc.descriptionWe present HST images at 622 nm and 300 nm of the optical jet in 3C273 and determine the run of the optical spectral index at 0.2" along the jet. We find no evidence for localized acceleration or loss sites, and support for a little-changing spectral shape throughout the jet. We consider this further evidence in favour of a distributed acceleration process.
dc.description4 pages, 2 figures, presented at "Particles and Fields in Radio Galaxies", Oxford, 2000 (to appear in ASP conf. series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0011413
dc.identifierhttp://arxiv.org/abs/astro-ph/0011413
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2074
dc.subjectAstrophysics
dc.titleA high-resolution multi-wavelength study of the jet in 3C 273
dc.typetext

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