On the possibility of faint molecular lines of PO, PH, MgH⁺, and CN in the solar spectrum

dc.contributor.author	Sinha, K.
dc.contributor.author	Tripathi, B. M.
dc.contributor.author	Atalla, R. M.
dc.contributor.author	Singh, P. D.
dc.date.accessioned	2010-02-15T04:49:48Z
dc.date.available	2010-02-15T04:49:48Z
dc.date.issued	1988
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/505
dc.description.abstract	Equivalent width calculations for some electronic and vibration-rotation transitions of the molecules PO, PH, MgH⁺, and CN have been carried out for a few umbral, photospheric, and facular model atmospheres. It appears that a few weak lines of these molecules might show up in the umbral spectrum. Le Blanc bands of CN are too weak for detection in the solar spectrum.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp115-221
dc.subject	Faint molecules lines - PO, PH, MgH⁺ and CN	en_US
dc.title	On the possibility of faint molecular lines of PO, PH, MgH⁺, and CN in the solar spectrum	en_US
dc.type	Article	en_US