Near infrared emission spectra of CoH and CoD

被引:13
|
作者
Gordon, Iouli E.
Le Roy, Robert J.
Bernath, Peter F. [1 ]
机构
[1] Univ Waterloo, Dept Phys, Waterloo, ON N2L 3G1, Canada
[2] Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
cobalt monohydride; Fourier transform spectroscopy; near infrared; spin-orbit splitting;
D O I
10.1016/j.jms.2006.02.011
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
New high resolution emission spectra of CoH and CoD molecules have been recorded in the 640 run to 3.5 mu m region using a Fourier transform spectrometer. The bands were excited in a carbon tube furnace by the reaction of cobalt metal vapor and a mixture of H-2 or D-2 With He at a temperature of about 2600 degrees C. Eight bands were observed for the A(t3)Phi(4)-X-3 Phi(4) electronic transition of CoD, and five bands for the corresponding transition of CoH. The (0,0) bands of the A(t3)Phi(3)-X-3 Phi(3) system Were also recorded for both isotopologues, although one of the parity components in the X-3 Phi(3) sub-state of CoH was found to be perturbed. The A(t3)Phi(3)-X-3 Phi(4) transition was also observed in our spectrum of CoH. In addition, a new [13.3]4 electronic state was found by observing [13.3]4-X-3 Phi(3) and [13.3]4-X-3 Phi(4) transitions in the spectrum of CoD. Analysis of the transitions with Delta Omega = 0, +/- 1 provided more accurate values of spin-orbit splittings between Omega = 4 and Omega = 3 components. The around-state data for both molecules were fitted both to band-constant and Dunham-expansion expressions, and a combined-isotopologue analysis of the X-3 Phi(4) spin component was carried out using the data for CoH and CoD. The tipper states Were represented by term values in these analyses because of perturbations, but estimated band constants for them were obtained in separate fits in which ground-state constants were held fixed. (C) 2006 Elsevier Inc. All rights reserved.
引用
收藏
页码:11 / 18
页数:8
相关论文
共 50 条
  • [41] DISCOVERY OF RUBIDIUM, CADMIUM, AND GERMANIUM EMISSION LINES IN THE NEAR-INFRARED SPECTRA OF PLANETARY NEBULAE
    Sterling, N. C.
    Dinerstein, Harriet L.
    Kaplan, Kyle F.
    Bautista, Manuel A.
    ASTROPHYSICAL JOURNAL LETTERS, 2016, 819 (01)
  • [42] Pathlength selection of determing tire chemical oxygen demand (COD) in wastewater by using near-infrared transmission spectra
    He Jin-Cheng
    Yang Xiang-Long
    Wang Li-Ren
    JOURNAL OF INFRARED AND MILLIMETER WAVES, 2007, 26 (04) : 317 - 320
  • [43] INFRARED-SPECTRA AND CIRCUMSTELLAR EMISSION OF LATE-TYPE STARS .4. NEAR-INFRARED SPECTRA OF S-TYPE STARS
    NOGUCHI, K
    KOBAYASHI, Y
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1993, 45 (01) : 85 - 96
  • [44] EMISSION SPECTRUM OF HCL IN THE NEAR INFRARED
    NEWMAN, R
    JOURNAL OF CHEMICAL PHYSICS, 1952, 20 (04): : 749 - 750
  • [45] Near infrared emission spectrum of HCN
    Mellau, Georg Ch.
    Winnewisser, Brenda P.
    Winnewisser, Manfred
    JOURNAL OF MOLECULAR SPECTROSCOPY, 2008, 249 (01) : 23 - 42
  • [46] NEAR-INFRARED EMISSION SPECTRUM OF NO
    HORN, EF
    DICKEY, FP
    JOURNAL OF CHEMICAL PHYSICS, 1964, 41 (06): : 1614 - &
  • [47] Near-infrared emission of protostars
    Calvet, N
    Hartmann, L
    Strom, SE
    ASTROPHYSICAL JOURNAL, 1997, 481 (02): : 912 - 917
  • [48] Millimeter-wave spectra of (H2COH+)-C-13 and D2COD+
    Dore, L
    Cazzoli, G
    Civis, S
    Scappini, F
    JOURNAL OF MOLECULAR SPECTROSCOPY, 1997, 183 (01) : 107 - 112
  • [49] ASTROPHYSICS - EMISSION-LINES IN NEAR-INFRARED SPECTRA OF 12 FAINT PLANETARY-NEBULAE
    ANDRILLAT, Y
    HOUZIAUX, L
    COMPTES RENDUS HEBDOMADAIRES DES SEANCES DE L ACADEMIE DES SCIENCES SERIE B, 1977, 285 (11): : 263 - &