Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...332..531b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 332, Sept. 1, 1988, p. 531-538.
Astronomy and Astrophysics
Astrophysics
93
Astrophysics, Cn Emission, Free Radicals, Gas Dissociation, Spectral Bands, Ground State, Nitric Oxide, Oscillator Strengths, Radiative Lifetime, Visible Spectrum
Scientific paper
The dissociation energy (D0) of CN is determined to be 7.65±0.06 eV. This corresponds to ΔHf(CN) = 105.3±1.5 kcal per mole. This result is obtained not only from extensive ab inition MRCI calculations using a very large Gaussian basis set, but also from extrapolation of the directly computed value by comparison of computed and experimental results for NO, C2, and N2. The lifetime of the υarcmin = 0 level of the violet (B2Σ+ → X2Σ+) system has been completed to be 62.4 ns. Lifetimes for the red (A2Π → X2Σ+) system decrease with increasing υarcmin, which is consistent both with recent experiment and calculations.
Bauschlicher Charles W. Jr.
Langhoff Stephen R.
Taylor Peter R.
No associations
LandOfFree
Theoretical study of the dissociation energy and the red and violet band systems of CN does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Theoretical study of the dissociation energy and the red and violet band systems of CN, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical study of the dissociation energy and the red and violet band systems of CN will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-909445