Novae and BAL QSOs: The Aluminum Test

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dc.creatorShields, Gregory A.
dc.date1997-06-30
dc.date.accessioned2026-07-07T02:23:42Z
dc.date.available2026-07-07T02:23:42Z
dc.descriptionNovae have been proposed as the explanation of high reported abundances of heavy elements in the gas producing the broad absorption lines (BALs) of QSOs. High abundances of odd numbered elements, including aluminum, are predicted. Available data contains hints that the Al/Si ratio may be high both in the BAL gas and in the broad emission-line gas.
dc.description6 pages LaTeX using paspconf.sty. To appear in Mass Ejection from Active Galactic Nuclei, N. Arav, I. Shlosman, and R. J. Weymann (Eds.), ASP Conf. Series, 1997, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9706301
dc.identifierhttp://arxiv.org/abs/astro-ph/9706301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11352
dc.subjectAstrophysics
dc.titleNovae and BAL QSOs: The Aluminum Test
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