Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1887
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dc.contributor.authorTrivedi, C-
dc.contributor.authorSinha, K-
dc.date.accessioned2007-10-16T06:58:21Z-
dc.date.available2007-10-16T06:58:21Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 1, pp. 87 - 91en
dc.identifier.urihttp://hdl.handle.net/2248/1887-
dc.description.abstractRather contrasting values of the oscillator strengths for the (0,0) band of SiH+ molecules for the A 1II - X1 capital sigma+ transition have been reported in the literature. We investigate these with the help of a new set of solar photospheric models, abundances and moleculer parameters. The results are found to be in agreement with the earlier solar studies.In view of the extremely weak nature of the SiH+ features, it appears probable to scale up the solar oscillator strengths by a factor of 2.en
dc.format.extent392355 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25...87Ten
dc.subjectOscillator strengthsen
dc.subjectPhotospheric spectrumen
dc.subjectNaini Talen
dc.titleOn the solar oscillator strength of SiH^{+}en
dc.typeArticleen
Appears in Collections:BASI Publications

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