Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5260
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dc.contributor.authorBaddi, Raju R.-
dc.date.accessioned2012-08-23T11:23:41Z-
dc.date.available2012-08-23T11:23:41Z-
dc.date.issued2012-02-
dc.identifier.citationAstronomical Journal, 2012, Vol.143, p26en
dc.identifier.issn0004-6256-
dc.identifier.issn1538-3881(Online)-
dc.identifier.urihttp://hdl.handle.net/2289/5260-
dc.descriptionRestricted Access An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractA survey of radio recombination lines in the Galactic plane with longitude -32° < l < +80° and latitude b < ±3° using Ooty Radio Telescope (ORT) at 328 MHz is reported. ORT observations were made using a New Digital Backend (NDB) recently added to the telescope. With the NDB ORT had a beam of 2fdg3 × 2fdg2 sec(δ) and a passband of ~1 MHz in the spectral line mode. The above-mentioned Galactic region was divided into ~2° × 2° patches with the ORT beam pointed to the center. The ORT observations form a study of the distribution of extended low-density warm-ionized medium (ELDWIM) in the inner Galaxy using H271α RLs. By obtaining kinematical distances using V LSR of the H271α RLs, the distribution of ELDWIM clouds within the inner Galaxy has been deduced for the region given above.en
dc.language.isoenen
dc.publisherIOP Publishing for the American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/2012AJ....143...26Ben
dc.relation.urihttp://arxiv.org/abs/1208.1167en
dc.relation.urihttp://dx.doi.org/10.1088/0004-6256/143/2/26en
dc.rights2012 American Astronomical Societyen
dc.subjectH II regionsen
dc.subjectISM: abundancesen
dc.subjectradio lines: ISMen
dc.titleSurvey of radio recombination lines using the Ooty radio telescope at 328 MHz in the inner galaxyen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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