J/A+A/577/L2ivo://CDS.VizieR/J/A+A/577/L2doi:10.26093/cds/vizier.35779002CDSGerin M.Pety J.Fuente A.Cernicharo J.Commercon B.Marcelino N.2015-09-09T10:55:57Z2015-05-12T08:01:21ZCDS support team

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

cds-question@unistra.frmolecular-cloudsradial-velocityIn the theory of star formation, the first hydrostatic core (FHSC) phase is a critical step in which a condensed object emerges from a prestellar core. This step lasts about one thousand years, a very short time compared with the lifetime of prestellar cores, and therefore is hard to detect unambiguously. We present IRAM Plateau de Bure observations of the Barnard 1b dense molecular core, combining detections of H2CO and CH3OH spectral lines and dust continuum at 2.3" resolution (~500AU). The two compact cores B1b-N and B1b-S are detected in the dust continuum at 2mm, with fluxes that agree with their spectral energy distribution. Molecular outflows associated with both cores are detected. They are inclined relative to the direction of the magnetic field, in agreement with predictions of collapse in turbulent and magnetized gas with a ratio of mass to magnetic flux somewhat higher than the critical value, {mu}~2-7. The outflow associated with B1b-S presents sharp spatial structures, with ejection velocities of up to ~7km/s from the mean velocity. Its dynamical age is estimated to be ~2000yr. The B1b-N outflow is smaller and slower, with a short dynamical age of ~1000yr. The B1b-N outflow mass, mass-loss rate, and mechanical luminosity agree well with theoretical predictions of FHSC. These observations confirm the early evolutionary stage of B1b-N and the slightly more evolved stage of B1b-S.2015A&A...577L...2Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/577/L2CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/577/L2https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/577/L2http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/577/L2https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/577/L2https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/577/L2http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/577/L2GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/577/L2/list (List of FITS datacubes)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/577/L2/list?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/577/L2/list?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/577/L2/list?GETtext/xml+votable180.050000true53.3387531.126110.0055555555555555566/860https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/577/L2?format=asciiOpticaldefaultJ/A+A/577/L2/listList of FITS datacubesNy[155] Number of pixels along Y-axismeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Center right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Center declination (J2000)degpos.eq.dec;meta.mainScale[0.49] Scale of the imagearcsec/pixinstr.scalefloatNx[155] Number of pixels along X-axismeta.numberintNz[150/618] Number of slicesmeta.numberintFreq[145.12/145.61] Central frequencyGHzem.freqdoubleV.minLower value of radial velocity intervalkm/sphys.velocfloatV.maxUpper value of radial velocity intervalkm/sphys.velocfloatdVChannel spacingm/sspect.resolutionfloatsizeSize of the fits fileKibytephys.size;meta.fitsintfitsDownload the FITS filemeta.ref.urlcharFileNameName of the FITS file in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the filemeta.title;meta.file