J/A+A/621/A111ivo://CDS.VizieR/J/A+A/621/A111doi:10.26093/cds/vizier.36210111CDSChantzos J.Spezzano S.Endres C.Bizzocchi L.Lattanzi V.Laas J.,Vasyunin A.Caselli P.2019-01-28T13:46:23Z2019-01-15T08:31:39ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsThe ketenyl radical, HCCO, has recently been detected in the ISM for the first time. Further astronomical detections of HCCO will help us understand its gas-grain chemistry, and subsequently revise the oxygen-bearing chemistry towards dark clouds. Moreover, its deuterated counterpart, DCCO, has never been observed in the ISM. HCCO and DCCO still lack of a broad spectroscopic investigation although they exhibit a significant astrophysical relevance. In this work we aim to measure the pure rotational spectra of the ground state of HCCO and DCCO in the millimeter and submillimeter region, considerably extending the frequency range covered by previous studies. The spectral acquisition was performed using a frequency-modulation absorption spectrometer between 170 and 650GHz. The radicals were produced in a low-density plasma generated from a select mixture of gaseous precursors. For each isotopologue we were able to detect and assign more than 100 rotational lines. The new lines have significantly enhanced the previous data set allowing the determination of highly precise rotational and centrifugal distortion parameters. In our analysis we have taken into account the interaction between the ground electronic state and a low-lying excited state (Renner-Teller pair) which enables the prediction and assignment of rotational transitions with Ka up to 4. The present set of spectroscopic parameters provides highly accurate, millimeter and submillimeter rest-frequencies of HCCO and DCCO for future astronomical observations. We also show that towards the pre-stellar core L1544, ketenyl peaks in the region where c-C_3_H_2_ peaks, suggesting that HCCO follows a predominant hydrocarbon chemistry, as already proposed by recent gas-grain chemical models.2019A&A...621A.111Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/621/A111CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/621/A111https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/621/A111http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/621/A111https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/621/A111https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/621/A111http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/621/A111GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/621/A111/table1Assignments, measured line positions and least-squares residuals for the analysed transitions of HCCONLower state Nphys.atmol.qnintN'Upper state Nphys.atmol.qnintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKa'Upper state Kaphys.mol.qnintKc'Upper state Kcphys.mol.qnintv'Upper state vphys.mol.qnintJ'Upper state Jphys.atmol.qnintF'Upper state Fphys.atmol.qnintKaLower state Kaphys.mol.qnintKcLower state Kcphys.mol.qnintvLower state vphys.mol.qnintJLower state Jphys.atmol.qnintFLower state Fphys.atmol.qnintObsMeasured line positionMHzem.freqdoubleO-CLeast-squares residualMHzstat.fit.residualdoubleuncAssumed uncertaintyMHzstat.errorfloatRefReference (G1)meta.ref;pos.framecharJ/A+A/621/A111/table2Assignments, measured line positions and least-squares residuals for the analysed transitions of DCCOrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintN'Upper state Nphys.atmol.qnintKa'Upper state Kaphys.mol.qnintKc'Upper state Kcphys.mol.qnintv'Upper state vphys.mol.qnintJ'Upper state Jphys.atmol.qnintNlower state Nphys.atmol.qnintKaLower state Kaphys.mol.qnintKcLower state Kcphys.mol.qnintvLower state vphys.mol.qnintJLower state Jphys.atmol.qnintObsMeasured line positionMHzem.freqdoubleO-CLeast-squares residualMHzstat.fit.residualdoubleuncAssumed uncertaintyMHzstat.errorfloatRefReference (G1)meta.ref;pos.framechar