On the oscillator strength and the dissociation energy of CN molecules

dc.contributor.author	Sinha, K
dc.contributor.author	Tripathi, B. M
dc.date.accessioned	2006-04-10T05:52:54Z
dc.date.available	2006-04-10T05:52:54Z
dc.date.issued	1986-03
dc.identifier.citation	BASI, Vol. 14, No. 1, pp. 40-44	en
dc.identifier.uri	http://hdl.handle.net/2248/905
dc.description.abstract	Equivalent widths of the CN red system in the solar spectrum are determined and compared with previous observational data in order to evaluate various published values for oscillator strength and dissociation energy. The Holweger and Mueller (1974) photospheric model with an oscillator strength of 1.9 x 10 to the -3rd and a CN dissociation energy between 7.66 and 7.76 is found to provide results consistent with the red system values observed in the photospheric spectrum. This range of dissociation energy values can also be used for the violet system without increasing UV opacity	en
dc.format.extent	347083 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	CN molecules	en
dc.subject	Solar spectrum	en
dc.title	On the oscillator strength and the dissociation energy of CN molecules	en
dc.type	Article	en