Mathematics
Scientific paper
Jun 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011mss..confetd02r&link_type=abstract
"International Symposium On Molecular Spectroscopy, 66th Meeting, Held 20-24 June, 2011 at Ohio State University. http://molspec
Mathematics
Electronic
Scientific paper
Emission spectra of the B2Σ+--X2Σ+ transition of 13C14N have been observed at high resolution using the Fourier transform spectrometer associated with the McMath-Pierce Solar Telescope of the National Solar Observatory. The spectra have been measured in the 21000--30000 cm-1 region and a total of 52 vibrational bands involving vibrational levels up to v=15 of the ground and excited states have been rotationally analyzed to provide a much improved set of spectroscopic constants. The results of the present analysis should prove useful in the identification of additional 13C14N lines in comets and cool stars, and will help in the determination of the 12C/13C abundance ratio. The observation of a number of highly-excited vibrational bands of the A2Π--X2Σ+ transition as well as a few bands of the B2Σ+--A2Π transition will also be reported.
Bernath Peter F.
Ram R. S.
No associations
LandOfFree
Fourier Transform Emission Spectroscopy of the B2Σ+--X2Σ+ (violet) System of 13C14N 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 Fourier Transform Emission Spectroscopy of the B2Σ+--X2Σ+ (violet) System of 13C14N, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fourier Transform Emission Spectroscopy of the B2Σ+--X2Σ+ (violet) System of 13C14N will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1001004