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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/976
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dc.contributor.authorAnantharamaiah, K.R.-
dc.contributor.authorZhao, J.H.-
dc.contributor.authorGoss, W.M.-
dc.contributor.authorViallefond, F.-
dc.date.accessioned2005-12-29T09:04:42Z-
dc.date.available2005-12-29T09:04:42Z-
dc.date.issued1995-
dc.identifier.citationJournal of Astrophysics and Astronomy Supplement, 1995, Vol. 16, p273 -274.en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2289/976-
dc.description.abstractUsing the Very Large Array1 and the Australia Telescope we have searched for the H92 α recombination line from 14 external galaxies and detected the line in 9 of them. All the detected galaxies have starburst nuclei and the line emission is only from the nuclear region. No line was detected in two well known Seyfert II galaxies that were searched to similar sensitivity levels.en
dc.format.extent84851 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectGalaxies;en
dc.subjectStar burst;en
dc.subjectSeyfert II;en
dc.subjectRadio recombination lines;en
dc.titleRadio recombination lines from external galaxiesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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