J/A+A/616/A66ivo://CDS.VizieR/J/A+A/616/A66doi:10.26093/cds/vizier.36160066CDSMoscadelli L.Rivilla V.M.Cesaroni R.Beltran M.T.Sanchez-Monge A.,Schilke P.Mottram J.C.Ahmadi A.Allen V.Beuther H.Csengeri T.,Etoka S.Galli D.Goddi C.Johnston K.G.Klaassen P.D.Kuiper R.,Kumar M.S.N.Maud L.T.Moller T.Peters T.Van der Tak F.Vig S.2019-11-11T22:00:00Z2019-02-01T13:06:11ZCDS support team

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

cds-question@unistra.frstar-forming-regionsastrophysical-masersradio-astronomyG24.78+0.08 is a well known high-mass star-forming region, where several molecular cores harboring OB young stellar objects are found inside a clump of size ~=1pc. This article focuses on the most prominent of these cores, A1, where an intense hypercompact (HC) HII region has been discovered by previous observations. Our aim is to determine the physical conditions and the kinematics of core A1, and study the interaction of the HII region with the parental molecular core. We combine ALMA 1.4mm high-angular resolution (~=0.2'') observations of continuum and line emission with multi-epoch Very Long Baseline Interferometry data of water 22GHz and methanol 6.7GHz masers. These observations allow us to study the gas kinematics on linear scales from 10 to 10^4^au, and to accurately map the physical conditions of the gas over core A1. The 1.4mm continuum is dominated by free-free emission from the intense HC HII region (size~=1000au) observed to the North of core A1 (region A1N). Analyzing the H30{alpha} line, we reveal a fast bipolar flow in the ionized gas, covering a range of LSR velocities (VLSR) of ~=60km/s. The amplitude of the VLSR gradient, 22km/s/mpc, is one of the highest so far observed towards HC HII regions. Water and methanol masers are distributed around the HC HII region in A1N, and the maser three-dimensional (3D) velocities clearly indicate that the ionized gas is expanding at high speed (>=200km/s) into the surrounding molecular gas. The temperature distribution (in the range 100-400K) over core A1, traced with molecular (CH_3_OCHO, ^13^CH_3_CN, ^13^CH_3_OH, and CH_3_CH_2_CN) transitions with level energy in the range 30K<=E_u_/k<=300K, reflects the distribution of shocks produced by the fast-expansion of the ionized gas of the HII region. The high-energy (550K<=E_u_/k<=800K) transitions of vibrationally excited CH_3_CN are likely radiatively pumped, and their rotational temperature can significantly differ from the kinetic temperature of the gas. Over core A1, the VLSR maps from both the 1.4mm molecular lines and the 6.7GHz methanol masers consistently show a VLSR gradient (amplitude ~=0.3km/s/mpc) directed approximately S-N. Rather than gravitationally supported rotation of a massive toroid, we interpret this velocity gradient as a relatively slow expansion of core A1.2018A&A...616A..66Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/616/A66CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/616/A66https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/616/A66http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/616/A66https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/616/A66https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/616/A66http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/616/A66GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/616/A66/tableb1 (6.7GHz CH_3_OH maser parameters for G24.78+0.08 A1)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/616/A66/tableb1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/616/A66/tableb1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/616/A66/tableb1?GETtext/xml+votable180.050000true279.0523439-7.20300310.0055555555555555566/30218https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/616/A66?format=asciiRadiodefaultJ/A+A/616/A66/tableb16.7GHz CH_3_OH maser parameters for G24.78+0.08 A1e_oDErms uncertainty on oDE (3)masstat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCluster[A1N A1SW CM] Cluster name or CM for Centers of Motionmeta.id.parentcharFeatFeature label numbermeta.idcharn_Feat[b] Note (1)meta.notecharEpochsObserving epochs at which the feature was detected (2)meta.codecharIpeak? Intensity of the strongest spot, averaged over the observing epochs at restfreq=6.668519GHzJy/beamphot.flux.density;em.radio.3-6GHzfloatnullableVLSRIntensity-weighted LSR velocity, averaged over the observing epochskm/sphys.veloc;pos.lsrfloatoRAPosition offset along RA (3)maspos.eq.ra;arith.difffloate_oRArms uncertainty on oRA (3)masstat.errorfloatoDEPosition offset along DE (3)maspos.eq.dec;arith.difffloatVx? Component of the relative proper motion along RA (4)km/sphys.veloc;pos.cartesian.xfloatnullablee_Vx? rms uncertainty on Vx (4)km/sstat.errorfloatnullableVy? Component of the relative proper motion along DE (4)km/sphys.veloc;pos.cartesian.yfloatnullablee_Vy? rms uncertainty on Vy (4)km/sstat.errorfloatnullable_RAComputed Right Ascension for Equinox: J2000degpos.eq.ra;meta.main_DEComputed Declination for Equinox: J2000degpos.eq.dec;meta.main