Dark Matter

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dc.creatorBahcall, Neta
dc.date1996-11-11
dc.date.accessioned2026-07-07T02:22:17Z
dc.date.available2026-07-07T02:22:17Z
dc.descriptionObservations in the optical, in X-rays, and gravitational lensing of galaxies, clusters of galaxies, and large-scale structure are beginning to provide clues to the dark matter problem. I review the impact of these observations on some of the main questions relating to dark matter: How much dark matter is there? Where is it located? What is the nature of the dark matter? and what is the amount of baryonic dark matter.
dc.descriptionFigures can be obtained by e-mail to neta@astro.princeton.edu
dc.identifierhttps://arxiv.org/abs/astro-ph/9611080
dc.identifierhttp://arxiv.org/abs/astro-ph/9611080
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10821
dc.subjectAstrophysics
dc.titleDark Matter
dc.typetext

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