J/A+A/507/1425ivo://CDS.VizieR/J/A+A/507/1425doi:10.26093/cds/vizier.35071425CDSVan Kempen T.A.Van Dishoeck E.F.Guesten R.Kristensen L.E.,Schilke P.Hogerheijde M.R.Boland W.Menten K.M.Wyrowski F.CDS support team

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

cds-question@unistra.frThe origin and heating mechanisms of warm (50<T<200K) molecular gas in low-mass young stellar objects (YSOs) are strongly debated. Both passive heating of the inner collapsing envelope by the protostellar luminosity as well as active heating by shocks and by UV associated with the outflows or accretion have been proposed. Most data so far have focussed on the colder gas component. We aim to characterize the warm gas within protosteller objects, and disentangle contributions from the (inner) envelope, bipolar outflows and the quiescent cloud. ************************************************************************** * * * Sorry, but the author(s) never supplied the tabular material * * announced in the paper * * * **************************************************************************2009A&A...507.1425Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/507/1425CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/507/1425https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/507/1425http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/507/1425https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/507/1425https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/507/1425http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/507/1425GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefault