Theoretical implications of microwave background radiation anisotropy experiments

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dc.creatorRocha, Graca
dc.creatorHancock, Stephen
dc.date1996-11-27
dc.date.accessioned2026-07-07T02:22:24Z
dc.date.available2026-07-07T02:22:24Z
dc.descriptionObservational results from several experiments such as COBE, SP, Saskatoon, PYTHON, ARGO, MAX, MSAM, Tenerife and CAT are considered and a comparison is made with predictions from several models. Conclusions are reached about the viability of current structure formation models.
dc.description7 pages LaTeX, including 6 PostScript figures. To appear in proceedings of the XXXIst Rencontre de Moriond, `Microwave Background Anisotropies'
dc.identifierhttps://arxiv.org/abs/astro-ph/9611228
dc.identifierhttp://arxiv.org/abs/astro-ph/9611228
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10862
dc.subjectAstrophysics
dc.titleTheoretical implications of microwave background radiation anisotropy experiments
dc.typetext

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