J/A+A/657/A99       The rotational spectrum of glycinamide       (Kisiel+, 2022)

Millimetre-wave laboratory study of glycinamide and search for it with ALMA toward Sagittarius B2(N). Kisiel Z., Kolesnikova L., Belloche A., Guillemin J.-C., Pszczolkowski L., Alonso E.R., Garrod R.T., Bialkowska-Jaworska E., Leon I., Mueller H.S.P., Menten K.M., Alonso J.L. <Astron. Astrophys. 657, A99 (2022)> =2022A&A...657A..99K 2022A&A...657A..99K (SIMBAD/NED BibCode)
ADC_Keywords: Interstellar medium ; Spectroscopy ; Atomic physics Keywords: astrochemistry - ISM: molecules - astronomical databases: miscellaneous - ISM: individual objects: Sagittarius B2 - line: identification Abstract: Glycinamide (NH2CH2C(O)NH2) is considered to be one of the possible precursors of the simplest amino acid glycine. Its only rotational spectrum reported so far has been in the cm-wave region on a laser-ablation generated supersonic expansion sample. The aim of this work is to extend the laboratory spectrum of glycinamide into the millimetre wave region to support its searches in the interstellar medium and to perform the first check for its presence in the high-mass star forming region Sagittarius B2(N). Glycinamide was synthesised chemically and was studied with broadband rotational spectroscopy in the 90-329 GHz region with the sample in slow flow at 50°C. Tunneling across a low energy barrier between two symmetry equivalent configurations of the molecule resulted in splitting of each vibrational state and many perturbations in associated rotational energy levels, requiring careful coupled state fits for each vibrational doublet. We searched for emission of glycinamide in the imaging spectral line survey ReMoCA performed with the Atacama Large Millimetre/submillimetre Array toward Sgr B2(N). The astronomical spectra were analysed under the assumption of local thermodynamic equilibrium. We report the first analysis of the mm-wave rotational spectrum of glycinamide, resulting in fitting to experimental measurement accuracy of over 1200 assigned and measured transition frequencies for the ground state tunneling doublet, of many lines for tunneling doublets for two singly excited vibrational states, and determination of precise vibrational separation in each doublet. We did not detect emission from glycinamide in the hot molecular core Sgr B2(N1S). We derived a column density upper limit of 1.5x1016cm-2, which implies that glycinamide is at least seven times less abundant than aminoacetonitrile and 1.8 times less abundant than urea in this source. Description: Observed rotational transitions of glycinamide in the ground state and two excited state tunneling doublets File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 119 1400 Fitted rotational transitions of glycinamide in the ground state (0+ 0- doublet) table6.dat 80 990 Fitted rotational transitions of glycinamide in v27=1 state (1+ 1- doublet) table7.dat 80 781 Fitted rotational transitions of glycinamide in v26=1 state (0+ 0- doublet) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.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 10- 12 I3 --- v' Upper state v quantum number (1) 15- 17 I3 --- J" Lower state J quantum number 18- 20 I3 --- Ka" Lower state Ka quantum number 21- 23 I3 --- Kc" Lower state Kc quantum number 24- 26 I3 --- v" Lower state v quantum number (1) 40- 50 F11.4 MHz FreqObs Observed transition frequency 53- 59 F7.4 MHz O-C Observed minus calculated frequency 62- 66 F5.3 MHz FreqExp Experimental uncertainty 69- 75 F7.4 MHz (O-C)b ? Observed minus calculated frequency for blends 77- 80 F4.2 --- wb ? Weight of the components of the blends 85-119 A35 --- Source Source of the data -------------------------------------------------------------------------------- Note (1): The vibrational quantum number v=0 corresponds to 0+ state and v=1 to 0- state of the ground state tunneling doublet. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.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 10- 12 I3 --- v' Upper state v quantum number (1) 15- 17 I3 --- J" Lower state J quantum number 18- 20 I3 --- Ka" Lower state Ka quantum number 21- 23 I3 --- Kc" Lower state Kc quantum number 24- 26 I3 --- v" Lower state v quantum number (1) 40- 50 F11.4 MHz FreqObs Observed transition frequency 53- 59 F7.4 MHz O-C Observed minus calculated frequency 62- 66 F5.3 MHz FreqExp Experimental uncertainty 69- 75 F7.4 MHz (O-C)b ? Observed minus calculated frequency for blends 77- 80 F4.2 --- wb ? Weight of the components of the blends -------------------------------------------------------------------------------- Note (1): The vibrational quantum number v=0 corresponds to 1+ state and v=1 to 1- state of the v27=1 tunneling doublet. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.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 10- 12 I3 --- v' Upper state v quantum number (1) 15- 17 I3 --- J" Lower state J quantum number 18- 20 I3 --- Ka" Lower state Ka quantum number 21- 23 I3 --- Kc" Lower state Kc quantum number 24- 26 I3 --- v" Lower state v quantum number (1) 40- 50 F11.4 MHz FreqObs Observed transition frequency 53- 59 F7.4 MHz O-C Observed minus calculated frequency 62- 66 F5.3 MHz FreqExp Experimental uncertainty 69- 75 F7.4 MHz (O-C)b ? Observed minus calculated frequency for blends 77- 80 F4.2 --- wb ? Weight of the components of the blends -------------------------------------------------------------------------------- Note (1): The vibrational quantum number v=0 corresponds to 0+ state and v=1 to 0- state of the v26=1 tunneling doublet. -------------------------------------------------------------------------------- Acknowledgements: Zbigniew Kisiel, kisiel(at)ifpan.edu.pl
(End) Z. Kisiel [IFPAN, Warszawa, Poland], P. Vannier [CDS] 29-Dec-2021
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