Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2583
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dc.contributor.authorAnantharamaiah, K.R.-
dc.contributor.authorNarayan, R.-
dc.date.accessioned2007-06-04T08:57:35Z-
dc.date.available2007-06-04T08:57:35Z-
dc.date.issued1988-
dc.identifier.citationRadio wave scattering in the interstellar medium; Proceedings of the AIP Conference, San Diego, CA, Jan. 18, 19, 1988, New York, American Institute of Physics, 1988, p185-189en
dc.identifier.urihttp://hdl.handle.net/2289/2583-
dc.descriptionRestricted Access.en
dc.description.abstractIt is argued that the enhanced scattering of radiowaves observed at low Galactic longitude and latitude is caused by the low-density outer envelopes of H II regions in the inner 8 kpc of the Galaxy. A simple phenomenological theory is developed to estimate the strength of density fluctuations in a turbulent medium and apply the theory to the H II envelopes, using the densities and sizes determined from a recent 325-MHz recombination-line survey. The predicted values are in good agreement with the observations.en
dc.format.extent241421 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Institute of Physicsen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1988AIPC..174..185Aen
dc.rights1988 American Institute of Physicsen
dc.subjectElectron density (Concentration)en
dc.subjectGalactic nuclei, H II regionsen
dc.subjectRadio scatteringen
dc.subjectInterstellar matteren
dc.subjectPower spectraen
dc.subjectPulsarsen
dc.subjectScintillationen
dc.titleThe origin of scattering in the inner galaxyen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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