The density profile and the wavelength dependence of compact radio source size

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dc.creatorPrigara, F. V.
dc.date2002-08-20
dc.date.accessioned2026-07-07T02:04:45Z
dc.date.available2026-07-07T02:04:45Z
dc.descriptionIn the gaseous disk model, the density profile is derived from the mass and energy conservation in the gravitational field of a central energy source. Using the condition for emission, following from the induced character of radiation process, we obtain the wavelength dependence of radio source size which is consistent with observational data.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0208360
dc.identifierhttp://arxiv.org/abs/astro-ph/0208360
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4878
dc.subjectAstrophysics
dc.titleThe density profile and the wavelength dependence of compact radio source size
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