Two Types of Radio Galaxies: A New Approach

dc.creatorEilek, Jean
dc.date2000-11-29
dc.date.accessioned2026-07-07T01:56:45Z
dc.date.available2026-07-07T01:56:45Z
dc.descriptionWe do not fully understand the dynamics and evolution of a radio galaxy. Models of classical double (Type II) sources are in a reasonable state, but these objects are rare. Non-type II sources (generically called Type I) are far more common, but much less well understood. In this paper I use the data to suggest possible new models for Type I sources, and discuss the physical questions which these new models raise.
dc.description8 pages, 2 figures, to appear in Particles and Fields in Radio Galaxies, ASP Conf. Series, eds. R. Laing and K. Blundell
dc.identifierhttps://arxiv.org/abs/astro-ph/0011550
dc.identifierhttp://arxiv.org/abs/astro-ph/0011550
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2114
dc.subjectAstrophysics
dc.titleTwo Types of Radio Galaxies: A New Approach
dc.typetext

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