The Swan system of C2:: A global analysis of Fourier transform emission spectra

被引:66
作者
Tanabashi, A.
Hirao, T.
Amano, T.
Bernath, P. F.
机构
[1] Ibaraki Univ, Inst Astrophys & Planetary Sci, Mito, Ibaraki, Japan
[2] Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada
[3] Univ Arizona, Dept Chem, Tucson, AZ 85721 USA
[4] Univ York, Dept Chem, York YO10 5DD, N Yorkshire, England
关键词
astrochemistry; ISM : clouds; ISM : molecules; methods : laboratory; molecular data; stars : late-type;
D O I
10.1086/510742
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The C-2 Swan system (d(3)Pi(g)-a(3)Pi(u)) was observed in emission for the Delta v = -3 to Delta v = +2 sequences in the 14,000-24,000 cm(-1) spectral range using a Fourier transform spectrometer. We carried out a global simultaneous fit by including a wide range of vibrational states. A total of 34 bands with v' = 0-10 and v '' = 0-9 were rotationally assigned. Numerous discrepancies were found in the assignments and in the measured transition wavenumbers between the new measurements and previous results. Most of the measured transition wavenumbers and their assignments for relatively low-v bands agreed with published data. On the contrary, for high-v bands our line positions and assignments disagreed with the tabulated literature values. In particular, the lines of six bands involving the levels with v' = 4, 5, and 6 are almost completely different from the previous work. Major sources of the disagreement are thought to be line congestion and perturbations found in these bands. From the analysis, perturbations for v' = 0, 1, 2, 4, 6, 8, 9, and 10 in the d(3)Pi(g) state were identified. A study of these rotational perturbations suggest that some of them are likely caused by interactions with high-v levels of the b (3)Sigma(-)(g) state.
引用
收藏
页码:472 / 484
页数:13
相关论文
共 55 条
[31]   INTER-STELLAR C2 MOLECULES TOWARD ZETA PERSEI [J].
HOBBS, LM .
ASTROPHYSICAL JOURNAL, 1979, 232 (03) :L175-L177
[32]  
HOBBS LM, 1982, ASTROPHYS J, V256, P108
[33]  
Huber K. P., 1979, MOL SPECTRA MOL STRU
[34]   THE 0.9-2.5 MICRON SPECTRUM OF COMET WEST-1976-VI [J].
JOHNSON, JR ;
FINK, U ;
LARSON, HP .
ASTROPHYSICAL JOURNAL, 1983, 270 (02) :769-777
[35]   MECHANISM FOR EXCITATION OF C2 HIGH-PRESSURE BANDS (C+C20-]C2(A3PI)+CO) [J].
KUNZ, C ;
HARTECK, P ;
DONDES, S .
JOURNAL OF CHEMICAL PHYSICS, 1967, 46 (10) :4157-&
[37]   HIGH-RESOLUTION SPECTRA OF C-2 SWAN BANDS FROM COMET WEST 1976-VI [J].
LAMBERT, DL ;
DANKS, AC .
ASTROPHYSICAL JOURNAL, 1983, 268 (01) :428-446
[38]   ORIGIN OF THE HIGH-PRESSURE BANDS OF C-2 [J].
LITTLE, CE ;
BROWNE, PG .
CHEMICAL PHYSICS LETTERS, 1987, 134 (06) :560-564
[39]   High resolution spectroscopy and spectral simulation of C2 using degenerate four-wave mixing [J].
Lloyd, GM ;
Ewart, P .
JOURNAL OF CHEMICAL PHYSICS, 1999, 110 (01) :385-392
[40]   EMISSION-BAND RATIOS IN COMET RUDNICKI (1966E) [J].
MAYER, P ;
ODELL, CR .
ASTROPHYSICAL JOURNAL, 1968, 153 (3P1) :951-&