Metallicity gradients as detectors of matter distribution in elliptical galaxies

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dc.creatorMartinelli, A.
dc.date1997-06-04
dc.date.accessioned2026-07-07T02:23:31Z
dc.date.available2026-07-07T02:23:31Z
dc.descriptionIn this work we discuss on the basis of the instantaneous recycling approximation the possibility of determining a relation between matter distribution (luminous and dark) in elliptical galaxies and the observed metallicity gradients. A particular case is developed in detail yielding an analitycal expression of the above relation.
dc.description4 pages, uses l-aa.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9706038
dc.identifierhttp://arxiv.org/abs/astro-ph/9706038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11277
dc.subjectAstrophysics
dc.titleMetallicity gradients as detectors of matter distribution in elliptical galaxies
dc.typetext

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