Holes in the Microwave Sky

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dc.creatorBartlett, J. G.
dc.creatorBlanchard, A.
dc.creatorBarbosa, D.
dc.creatorOukbir, J.
dc.date1997-07-06
dc.date.accessioned2026-07-07T02:23:45Z
dc.date.available2026-07-07T02:23:45Z
dc.descriptionWe discuss the implications of two possible, recent Sunyaev-Zel'dovich (SZ) detections for which no optical or X--ray counterparts have been found. This suggests that the objects reside at high redshift, which is difficult to reconcile with a critical cosmology. We develop this argument and find that an open model with $\Omo=0.2$ remains consistent with what we currently know about the two objects. The reasoning also demonstrates the utility of SZ cluster searches.
dc.descriptionProceedings of the PPEUC conference held in Cambridge, UK, April 7-11, 1997
dc.identifierhttps://arxiv.org/abs/astro-ph/9707059
dc.identifierhttp://arxiv.org/abs/astro-ph/9707059
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11369
dc.subjectAstrophysics
dc.titleHoles in the Microwave Sky
dc.typetext

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