On the search for BF, BH and BS molecular lines in sunspot spectra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4447

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DC Field	Value	Language
dc.contributor.author	Karthikeyan, B	-
dc.contributor.author	Bagare, S. P	-
dc.contributor.author	Rajamanickam, N	-
dc.contributor.author	Raja, V	-
dc.date.accessioned	2009-04-08T10:51:22Z	-
dc.date.available	2009-04-08T10:51:22Z	-
dc.date.issued	2009-02	-
dc.identifier.citation	Astroparticle Physics, Vol. 31, No. 1, pp. 6 - 12	en
dc.identifier.issn	0927-6505	-
dc.identifier.uri	http://hdl.handle.net/2248/4447	-
dc.description	Restricted Access	-
dc.description.abstract	A search has been carried out for the presence of rotational lines of boron containing diatomic molecules BF, BH and BS in the high resolution Fourier Transform Spectra of sunspots observed at the National Solar Observatory in Kitt Peak. The spectra were examined for a large number of rotational lines due to nine bands of BF, ten bands of BH and eight bands of BS in the range 9600–25,500 cm/sup−1. The presence of the lines due to six bands of BF and five bands of BS is confirmed. However, the presence of BH is found to be questionable. Equivalent widths have been measured for well resolved lines of BF and BS and effective rotational temperatures have been estimated.	en
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/10.1016/j.astropartphys.2008.10.009	en
dc.rights	© Elsevier	en
dc.subject	Sunspots	en
dc.subject	Line identification	en
dc.title	On the search for BF, BH and BS molecular lines in sunspot spectra	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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