A Model For The WMAP Anomalous Ecliptic Plane Signal

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dc.creatorSharpe, H. N.
dc.date2009-04-10
dc.date.accessioned2026-07-07T13:02:27Z
dc.date.available2026-07-07T13:02:27Z
dc.descriptionA simple model is presented to explain the high Galactic latitude anomalies in the WMAP data recently reported by Diego et al (2009). It is suggested that the anomalous deviation from a thermal spectrum could be caused by the propagation of background thermal radiation through a foreground optically thin HII cloud. The background radiation may be the remnant of cooling radio lobes associated with once-active jets from Sgr A*.
dc.description4 pages. Feedback welcomed please!
dc.identifierhttps://arxiv.org/abs/0904.1697
dc.identifierhttp://arxiv.org/abs/0904.1697
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226453
dc.subjectAstrophysics of Galaxies
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleA Model For The WMAP Anomalous Ecliptic Plane Signal
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