𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The X2 2Π12→X1 2Π32 electronic transitions of tellurium monohalides in the near infrared

✍ Scribed by E.H. Fink; K.D. Setzer; D.A. Ramsay; M. Vervloet


Publisher
Elsevier Science
Year
1991
Tongue
English
Weight
287 KB
Volume
177
Category
Article
ISSN
0009-2614

No coin nor oath required. For personal study only.

✦ Synopsis


Emission spectra of the O-O bands of the transitions X, *II ,,z+X, 2lI3,1 between the fine-structure components of the X'rI, ground states of TeF, TeCl, TeBr and TeI have been observed in the near-infrared spectral region between 2.35 and 2.5 pm. The X22n,,2 states of the radicals were excited by addition of halogens to the reaction system of microwavedischarged H2 with tellurium powder in a fast-flow system. The fine-structure splittings of the X 'Hi ground states were found to be 4187k 1 cm-' (TeF), 4022Srf I cm-' (TeCl), 4067k 3 cm-' (TeBr) and 41304 10 cm-' (TeI).


📜 SIMILAR VOLUMES


The Near-Infrared Y2Σ+–X2Π Transition of
✍ L.C. O'Brien; A.K. Lambeth; C.R. Brazier 📂 Article 📅 2002 🏛 Elsevier Science 🌐 English ⚖ 208 KB

The near-infrared Y 2 + -X 2 transition of the diatomic molecule CuSe was observed for the first time. A King-type carbon tube furnace was used to produce the gas phase of the CuSe molecules. The Fourier transform spectrometer associated with the National Solar Observatory, Kitt Peak, Arizona was us

The Near-InfraredY2Σ+–X2Π Transition of
✍ L.C. O'Brien; M. Dulick; S.P. Davis 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 75 KB

The near-infrared electronic transition of CuS has been observed for the first time. The spectrum of the Y 2 ⌺ ϩ -X 2 ⌸ transition, labeled by analogy with the CuO near infrared electronic transition, was recorded with the Fourier transform spectrometer associated with the McMath-Pierce Solar Telesc

The X12Π3/2 and X22Π1/2 Potential Energy
✍ Charles E. Miller; Brian J. Drouin 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 154 KB

The X(1)(2)Pi(3/2) and X(2)(2)Pi(1/2) potential energy curves of the FO free radical have been determined from a fit to the available high-resolution spectroscopic data. The data set spans the vibrational states v = 0-7 and includes X(2)(2)Pi(1/2) <-- X(1)(2)Pi(3/2) fine-structure transitions. The d