J/A+A/494/977ivo://CDS.VizieR/J/A+A/494/977doi:10.26093/cds/vizier.34940977CDSGerin M.Goicoechea J.R.Pety J.Hily-Blant P.CDS support team

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

cds-question@unistra.frFar-UV photons (FUV) strongly affect the physical and chemical state of molecular gas in the vicinity of young massive stars. Finding molecular tracers of the presence of FUV radiation fields in the millimeter wavelength domain is desirable because IR diagnostics (for instance PAHs) are not easily accessible along high extinction line-of-sights. Furthermore, gas phase diagnostics provide information on the velocity fields.2009A&A...494..977Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/494/977CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/494/977https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/494/977http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/494/977https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/494/977https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/494/977http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/494/977GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefault