Galactic Free-free and H-alpha Emission

dc.creatorSmoot, George F.
dc.date1998-01-13
dc.date1998-01-14
dc.date.accessioned2026-07-07T02:25:48Z
dc.date.available2026-07-07T02:25:48Z
dc.descriptionThis document provides a brief summary estimate of Galactic free-free emission and H-alpha emission and their relationship. Particular emphasis is placed on estimating the potential free-free emission in the region of significant confusion for CMB anisotropy measurements. Existing x-ray, ultraviolet and H$α$ emission provide limits on the radio free-free emission and vice versa. These limits are generally somewhat smaller than the observed ``free-free'' (signal proportional to frequency^{-2.15}) microwave signal. If this remains true, then some previously neglected source may be present. Physics argues that H-alpha emission is still the best tracer for Galactic free-free emission and thus a tool for diagnosing if there is a previously neglected emssion source.
dc.description10 pages including 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9801121
dc.identifierhttp://arxiv.org/abs/astro-ph/9801121
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12020
dc.subjectAstrophysics
dc.titleGalactic Free-free and H-alpha Emission
dc.typetext

Files

Collections