Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4437
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dc.contributor.authorShanmugavel, R-
dc.contributor.authorBagare, S. P-
dc.contributor.authorRajamanickam, N-
dc.contributor.authorBalachandra Kumar, K-
dc.date.accessioned2009-03-30T16:49:48Z-
dc.date.available2009-03-30T16:49:48Z-
dc.date.issued2008-06-
dc.identifier.citationSerbian Astronomical Journal, No. 176, pp. 51 - 58en
dc.identifier.issn1450-698X-
dc.identifier.urihttp://hdl.handle.net/2248/4437-
dc.description.abstractA high resolution spectrum of FTS sunspot umbra of NSO/Kitt Peak was used to conduct a search for the molecular absorption lines due to BeH, BeD and BeT isotopomers. Analysis led to estimates of identification of the molecular lines of bands A - X (0,0), (1,1) and (2,2) for BeH, A - X (0,0), (1,1), (2,2) and (3,3) for BeD and of A - X (0,0), (1,1) and (2,2) for BeT. Among the identified lines, those which are well resolved were selected for measurements to calculate equivalent widths. The values of effective rotational temperature T were estimated for bands A - X(1,1) and (2,2) of BeH, A - X(1,1) of BeD and A - X(2,2) of BeT to be 4228K, 4057K, 3941K and 3243K respectively.en
dc.language.isoenen
dc.publisherAstronomical Observatory, Serbiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2008SerAJ.176...51Sen
dc.relation.urihttp://dx.doi.org/10.2298/SAJ0876051Sen
dc.rights© Astronomical Observatory, Serbiaen
dc.subjectSunspotsen
dc.subjectLine: Identificationen
dc.titleIdentification of beryllium hydride isotopomer lines in sunspot umbral spectraen
dc.typeArticleen
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