High-resolution infrared spectrum and rovibrational analysis of the ν3 fundamental of diazirine,H213CN2

The high-resolution infrared spectrum of ¹³C-diazirine was recorded using a high-information Fourier transform spectrometer with a resolution of 0.0054 cm^?1. The rovibrational structure of the ν₃ fundamental at 1458.1884 cm^?1, which is an A-type parallel band (¹³CH₂ deformation) was assigned and analyzed with extensive use of modern methods of spectrum simulation. The rovibrational assignment and the molecular constants determined for the excited vibrational level of this band are given.     

The torsion-rotation microwave spectrum of 12CH318OH and the structure of methanol

The microwave and millimeter wave spectrum of ¹²CH₃¹⁸OH has been observed in the frequency region 7.9–200 GHz. Both a- and b-type transitions have been assigned and measured. This spectrum was analyzed using the method of Lees and Baker, and rotational constants, torsional constants, centrifugal distortion constants, the barrier to internal rotation and moments of inertia have been evaluated. The barrier has been found to be 374.91 ± 0.18 cm^?1, in good agreement with that of ¹²CH₃¹⁶OH. The moments of inertia were combined with those of other isotopic species to give a full substitution structure. To assist searches for this molecule in interstellar space a table of predicted frequencies of astrophysically interesting transitions is presented.     

Ground state spectroscopic constants of H15NCS,HN13CS,and HNC34S,and the molecular structure of isothiocyanic acid

The rotational spectrum of isothiocyanic acid was measured for the isotopically enriched species H¹⁵NCS and HN¹³CS as well as HNC³⁴S in natural abundance. In the frequency range from 8 to 240 GHz the a-type R-branch transitions were measured for all three isotopic species. The ^qQ₁ transitions were identified in the microwave region for H¹⁵NCS and HN¹³CS. The rotational and centrifugal distortion constants were determined using Watson's Hamiltonian in the S reduction, extended empirically to higher order terms in the angular momentum. The molecular structure of isothiocyanic acid was reevaluated using a modified substitution method and the NCS chain was found to be bent: $\text{r(}\text{NH}\text{) = 0.993}\text{A}\text{?}$, $\text{r(}\text{NC}\text{) = 1.207}\text{A}\text{?}$, $\text{r(}\text{CS}\text{) = 1.5665}\text{A}\text{?}$, ∠HNC = 131.7°, and ∠NCS = 173.8°. The molecule has the trans conformation.     

Absorption spectrum of deuterated hydrazoic acid, DN3 in the microwave and millimeterwave regiont

Thirty b-type P, Q and R branch rotational transitions and nineteen a-type Q and R branch transitions have been detected and measured for the slightly asymmetric rotor molecule D¹⁴N₃ in the frequency range from 8 to 340 GHz. The information obtained from the analysis of the observed frequencies are greatly improved values of the K-dependent parameters A_O = 344746.589(64) MHz, and D_K = 92.242(33) MHz, refined values for the rotational constants B_O and C_O, a complete set of quartic centrifugal distortion constants and several sextic distortion constants. Both a and b components of the electric dipole moment were determined giving a total dipole moment of μ = 1.76(5) debye.     

Gas-phase detection of HSOH: synthesis by flash vacuum pyrolysis of di-tert-butyl sulfoxide and rotational-torsional spectrum

Gas-phase oxadisulfane (HSOH), the missing link between the well-known molecules hydrogen peroxide (HOOH) and disulfane (HSSH), was synthesized by flash vacuum pyrolysis of di-tert-butyl sulfoxide. Using mass spectrometry, the pyrolysis conditions have been optimized towards formation of HSOH. Microwave spectroscopic investigation of the pyrolysis products allowed-assisted by high-level quantum-chemical calculations--the first measurement of the rotational-torsional spectrum of HSOH. In total, we have measured approximately 600 lines of the rotational-torsional spectrum in the frequency range from 64 GHz to 1.9 THz and assigned some 470 of these to the rotational-torsional spectrum of HSOH in its ground torsional state. Some 120 out of the 600 lines arise from the isotopomer H(34)SOH. The HSOH molecule displays strong c-type and somewhat weaker b-type transitions, indicating a nonplanar skew chain structure, similar to the analogous molecules HOOH and HSSH. The rotational constants (MHz) of the main isotopomer (A=202 069, B=15 282, C=14 840), determined by applying a least-squares analysis to the presently available data set, are in excellent agreement with those predicted by quantum-chemical calculations (A=202 136, B=15 279, C=14 840). Our theoretical treatment also derived the following barrier heights against internal rotation in HSOH (when in the cis and trans configurations) to be V(cis) approximately equal to 2216 cm(-1) and V(trans) approximately equal to 1579 cm(-1). The internal rotational motion results in detectable torsional splittings that are dependent on the angular momentum quantum numbers J and K(a).     

Spectroscopy among the stars

The space between the stars is not void, but filled with interstellar matter, mainly composed of dust and gas, which gather in large interstellar clouds. In our Galaxy these interstellar clouds are distributed along a thin, but extended layer which basically traces out the spiral distribution of matter: the stars, the gas, and the dust component. Up to the present time more than 100 different molecules have been identified in interstellar molecular clouds. The majority of the interstellar molecules constitute carbon containing organic substances. During the past years, overwhelming evidence has been gathered, mainly through spectroscopic observations, that interstellar molecular clouds provide the birthplaces for stars. In fact detailed high spectral and spatial resolution spectroscopic measurements reveal physical and chemical processes of the intricate star formation process.     

A precise study of the rotational spectrum of formaldehyde H212C16O,H213C16O,H212C18O,H213C18O

The rotational spectra of formaldehyde, H₂¹²C¹⁶O and its isotopic species H₂¹³C¹⁶O, H₂¹²C¹⁸O, and H₂¹³C¹⁸O have been investigated in the ground vibrational state in the frequency region between 8 and 460 GHz. For most cases in which measurements of the a-type R- and Q-branch transitions already existed the accuracy of the line position has been improved to about 10 kHz. For H₂¹²C¹⁶O and H₂¹³C¹⁶O a large number of ΔK_a = ±2 transitions were measured with similar accuracy. These new data when combined with all other available data and appropriate weightings lead to a set of ground state parameters which for the first time are compatible with infrared and ultraviolet data. The rotational constants (and 3σ standard deviations) obtained using Watson's A-reduced Hamiltonian are:

     

100.

Rotational Spectra of the Thiosulfeno Radical, HSS and DSS, between 0.3 and 0.9 THz     

Tanimoto M  Klaus T  Müller HS  Winnewisser G 《Journal of Molecular Spectroscopy》2000,199(1):73-80

The rotational spectra of the HSS and DSS radicals were studied in selected regions between 331 and 883 GHz. The radicals were produced by discharging a gaseous mixture of hydrogen (or deuterium) and hydrogen sulfide in the cell. The observation of the b-type Q-branch and R-branch lines with K(a) = 2-1 and 3-2 for HSS and DSS, respectively, as well as the a-type R-branch lines allowed the improvement and the determination of the molecular constants among them (in MHz) We have reevaluated the harmonic force field of HSS and the ground state average and approximate equilibrium structural parameters. For the latter, we obtained r(HS) = 135.23 pm, r(SS) = 196.03 pm, and angle = 101.74 degrees. These results are compared with those from previous and own quantum chemical calculations as well as with results of related molecules. Copyright 2000 Academic Press.     

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	H212C16O	H213C16O	H212C18O	H213C18O
A/MHz	281 970.572 (24)	281 993.258(135)	281 961.94 (39)	281 985.00 (93)
B/MHz	38 836.0456(13)	37 811.0887(25)	36 904.1693(66)	35 859.256(10)
C/MHz	34 002.2034(12)	33 213.9790(25)	32 511.5311(63)	31 697.868(10)

Rotational Spectra of the Thiosulfeno Radical, HSS and DSS, between 0.3 and 0.9 THz

The rotational spectra of the HSS and DSS radicals were studied in selected regions between 331 and 883 GHz. The radicals were produced by discharging a gaseous mixture of hydrogen (or deuterium) and hydrogen sulfide in the cell. The observation of the b-type Q-branch and R-branch lines with K(a) = 2-1 and 3-2 for HSS and DSS, respectively, as well as the a-type R-branch lines allowed the improvement and the determination of the molecular constants among them (in MHz) We have reevaluated the harmonic force field of HSS and the ground state average and approximate equilibrium structural parameters. For the latter, we obtained r(HS) = 135.23 pm, r(SS) = 196.03 pm, and angle = 101.74 degrees. These results are compared with those from previous and own quantum chemical calculations as well as with results of related molecules. Copyright 2000 Academic Press.