On the solar oscillator strength of SiH^{+}

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1887

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DC Field	Value	Language
dc.contributor.author	Trivedi, C	-
dc.contributor.author	Sinha, K	-
dc.date.accessioned	2007-10-16T06:58:21Z	-
dc.date.available	2007-10-16T06:58:21Z	-
dc.date.issued	1997	-
dc.identifier.citation	BASI, Vol. 25, No. 1, pp. 87 - 91	en
dc.identifier.uri	http://hdl.handle.net/2248/1887	-
dc.description.abstract	Rather 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.extent	392355 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1997BASI...25...87T	en
dc.subject	Oscillator strengths	en
dc.subject	Photospheric spectrum	en
dc.subject	Naini Tal	en
dc.title	On the solar oscillator strength of SiH^{+}	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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