Non-Explosive Hydrogen Burning: Where Do We Stand?

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dc.creatorArnould, M.
dc.creatorMowlavi, N.
dc.creatorChampagne, A.
dc.date1995-12-06
dc.date.accessioned2026-07-07T02:20:32Z
dc.date.available2026-07-07T02:20:32Z
dc.descriptionThe impact of nuclear physics uncertaintites on the abundances predicted to emerge from the cold CNO, NeNa and MgAl modes of hydrostatic hydrogen burning is discussed in the framework of a simple parametric model. In addition of being able to mimic qualitatively detailed stellar model predictions, these parametric calculations have the virtue of isolating in a crystal-clear way abundance uncertainties of purely nuclear physics origin.
dc.description13 pages, ps file (gziped + uuencoded), figures included. Review paper presented at the 32nd Liege Int. Astroph. Coll., "Stellar evolution: What Should Be Done?"
dc.identifierhttps://arxiv.org/abs/astro-ph/9512027
dc.identifierhttp://arxiv.org/abs/astro-ph/9512027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10238
dc.subjectAstrophysics
dc.titleNon-Explosive Hydrogen Burning: Where Do We Stand?
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