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	2010-02-09T07:12:37Z
dc.date.available	2010-02-09T07:12:37Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/496
dc.description.abstract	We compute the equivalent widths of CN red system in the solar spectrum and compare them with the observational data, in order to choose between various published oscillator strengths (f₀ ̠ ₀) and values of dissociation energy (D₀̊ ). It is found that the Holweger Muller (1974) photospheric model, along with f₀ ̠ ₀ = 1.9 x 10⁻ ³ and 7.66 ˂ D₀̊ (CN) ˂ 7.76 eV, gives results consistent with the red system observed in the photospheric spectrum. The same range of dissociation energy can also be used for the violet system without involving increased UV opacity.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi14-40
dc.subject	CN molecules, Solar Spectrum	en_US
dc.title	On the oscillator strength and the dissociation energy of CN molecules	en_US
dc.type	Article	en_US