J/A+A/666/A50       Rotational spectrum of vinylisocyanate        (Vavra+, 2022)

Millimeter wave spectrum and search for vinyl isocyanate toward Sgr B2(N) with ALMA. Vavra K., Kolesnikova L., Belloche A., Garrod R.T., Koucky J., Uhlikova T., Lukova K., Guillemin J.-C., Kania P., Muller H.S.P., Menten K.M., Urban S. <Astron. Astrophys. 666, A50 (2022)> =2022A&A...666A..50V 2022A&A...666A..50V (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics ; Interstellar medium ; Spectroscopy Keywords: astrochemistry - ISM: molecules - line: identification - ISM: individual objects: Sagittarius B2 - methods: laboratory: molecular Abstract: The interstellar detections of isocyanic acid (HNCO), methyl isocyanate (CH3NCO), and very recently also ethyl isocyanate (C2H5NCO) invite the question of whether or not vinyl isocyanate (C2H3NCO) can be detected in the interstellar medium. There are only low-frequency spectroscopic data (<40GHz) available for this species in the literature, which makes predictions at higher frequencies rather uncertain, which in turn hampers searches for this molecule in space using millimeter (mm) wave astronomy. The aim of the present study is on one hand to extend the laboratory rotational spectrum of vinyl isocyanate to the mm wave region and on the other to search, for the first time, for its presence in the high-mass star-forming region Sgr B2, where other isocyanates and a plethora of complex organic molecules are observed. We recorded the pure rotational spectrum of vinyl isocyanate in the frequency regions 127.5-218 and 285-330GHz using the Prague mm wave spectrometer. The spectral analysis was supported by high-level quantum-chemical calculations. On the astronomy side, we assumed local thermodynamic equilibrium to compute synthetic spectra of vinyl isocyanate and to search for it in the ReMoCA survey performed with the Atacama Large Millimeter/submillimeter Array (ALMA) toward the high-mass star-forming protocluster Sgr B2(N). Additionally, we searched for the related molecule ethyl isocyanate in the same source. Accurate values for the rotational and centrifugal distortion constants are reported for the ground vibrational states of trans and cis vinyl isocyanate from the analysis of more than 1000 transitions. We report nondetections of vinyl and ethyl isocyanate toward the main hot core of Sgr B2(N). We find that vinyl and ethyl isocyanate are at least 11 and 3 times less abundant than methyl isocyanate in this source, respectively. Although the precise formation mechanism of interstellar methyl isocyanate itself remains uncertain, we infer from existing astrochemical models that our observational upper limit for the CH3NCO:C2H5NCO ratio in Sgr B2(N) is consistent with ethyl isocyanate being formed on dust grains via the abstraction or photodissociation of an H atom from methyl isocyanate, followed by the addition of a methyl radical. The dominance of such a process for ethyl isocyanate production, combined with the absence of an analogous mechanism for vinyl isocyanate, would indicate that the ratio C2H3NCO:C2H5NCO should be less than unity. Even though vinyl isocyanate was not detected toward Sgr B2(N), the results of this work represent a significant improvement on previous low-frequency studies and will help the astronomical community to continue searching for this species in the Universe. Description: List of measured transitions of trans and cis vinyl isocyanate. JPL/CDMS catalog line list for trans and cis vinyl isocyanate. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea2.dat 100 520 List of the measured transitions of trans vinyl isocyanate tablea3.dat 102 892 List of the measured transitions of cis vinyl isocyanate tablea5.dat 73 6876 JPL/CDMS catalog line list for trans vinyl isocyanate tablea6.dat 73 5279 JPL/CDMS catalog line list for cis vinyl isocyanate -------------------------------------------------------------------------------- Byte-by-byte Description of file:tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- J' Upper state J quantum number 4- 6 I3 --- Ka' Upper state Ka quantum number 7- 9 I3 --- Kc' Upper state Kc quantum number 12- 14 I3 --- J" Lower state J quantum number 15- 17 I3 --- Ka" Lower state Ka quantum number 18- 20 I3 --- Kc" Lower state Kc quantum number 33- 43 F11.4 MHz FreqObs Observed transition frequency 46- 52 F7.4 MHz O-C Observed minus calculated frequency 55- 59 F5.3 MHz e_Freq Experimental uncertainty 62- 68 F7.4 MHz (O-C)b ? Observed minus calculated frequency for blends 70- 73 F4.2 --- wb ? Weight of the components of the blends 81-100 A20 --- Notes Source of the data (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 3 I2 --- J' Upper state J quantum number 5- 6 I2 --- Ka' Upper state Ka quantum number 8- 9 I2 --- Kc' Upper state Kc quantum number 13- 14 I2 --- J" Lower state J quantum number 16- 17 I2 --- Ka" Lower state Ka quantum number 19- 20 I2 --- Kc" Lower state Kc quantum number 33- 43 F11.4 MHz FreqObs Observed transition frequency 46- 52 F7.4 MHz O-C Observed minus calculated frequency 55- 59 F5.3 MHz e_Freq Experimental uncertainty 62- 68 F7.4 MHz (O-C)b ? Observed minus calculated frequency for blends 70- 73 F4.2 --- wb ? Weight of the components of the blends 81-102 A22 --- Notes Source of the data (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 13 F11.4 MHz Freq Frequency (1) 16- 21 F6.4 MHz e_Freq Uncertainty of the frequency 23- 29 F7.4 [nm2.MHz] log(Int) Base 10 logarithm of the integrated intensity in units of nm2 MHz at 300K 31 I1 --- DR Degrees of freedom in the rotational partition function 33- 41 F9.4 cm-1 Elow Energy of the lower level 42- 44 I3 --- gupp Upper state degeneracy 47- 51 I5 --- TAG Species tag or molecular identifier 53- 55 I3 --- QNFMT Format of the quantum numbers 56- 57 A2 --- J' Upper state J quantum number 58- 59 I2 --- Ka' Upper state Ka quantum number 60- 61 A2 --- Kc' Upper state Kc quantum number 68- 69 A2 --- J" Lower state J quantum number 70- 71 I2 --- Ka" Lower state Ka quantum number 72- 73 A2 --- Kc" Lower state Kc quantum number -------------------------------------------------------------------------------- Note (1): The key parameters used in the generation of this table: mu_a = 2.047 D, mu_b = 0.824 D, T = 300 K, and Qrot = 62500.3370 which takes into account the ground vibrational states of both isomers. Predictions of a-type transitions should be reliable up to J = 68 for Ka = 0 - 5 and J = 44 for Ka = 6, which correspond to the data sets encompassed in this work and interpolations between them. Predictions with Ka > 6 are not recommended for use and Ka < 6 beyond 330 GHz should be viewed with caution due to possible perturbations. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 13 F11.4 MHz Freq Frequency (2) 15- 21 F7.4 MHz e_Freq Uncertainty of the frequency 23- 29 F7.4 [nm2.MHz] log(Int) Base 10 logarithm of the integrated intensity in units of nm2 MHz at 300K 31 I1 --- DR Degrees of freedom in the rotational partition function 33- 41 F9.4 cm-1 Elow Energy of the lower level 42- 44 I3 --- gupp Upper state degeneracy 47- 51 I5 --- TAG Species tag or molecular identifier 53- 55 I3 --- QNFMT Format of the quantum numbers 56- 57 I2 --- J' Upper state J quantum number 58- 59 I2 --- Ka' Upper state Ka quantum number 60- 61 I2 --- Kc' Upper state Kc quantum number 68- 69 I2 --- J" Lower state J quantum number 70- 71 I2 --- Ka" Lower state Ka quantum number 72- 73 I2 --- Kc" Lower state Kc quantum number -------------------------------------------------------------------------------- Note (2): The key parameters used in the generation of this table: mu_a = 2.14 D, mu_b = 0.09 D, T = 300 K, Qrot = 62500.3370 which takes into account the ground vibrational states of both isomers, and E = 301 cm-1. -------------------------------------------------------------------------------- Global notes: Note (G1): References as follows: Kirby & Kroto (1978): 1978, J. Mol. Spectrosc., 70, 216. Bouchy & Roussy (1977): 1977, J. Mol. Spectrosc., 68, 156. -------------------------------------------------------------------------------- Acknowledgements: Lucie Kolesnikova, lucie.kolesnikova(at)vscht.cz
(End) L. Kolesnikova [UCT Prague, Czech Republic], P. Vannier [CDS] 26-Sep-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line