J/A+A/594/A59ivo://CDS.VizieR/J/A+A/594/A59doi:10.26093/cds/vizier.35940059CDSRiviere-Marichalar P.Merin B.Kamp I.Eiroa C.Montesinos B.2018-08-31T08:13:04Z2016-10-13T08:08:33ZCDS support team

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

cds-question@unistra.frinfrared-sourcesyoung-stellar-objectsGas plays a major role in the dynamical evolution of young stellar objects (YSOs). Its interaction with the dust is the key to our understanding planet formation later on in the protoplanetary disc stage. Studying the gas content is therefore a crucial step towards understanding YSO and planet formation. Such a study can be made through spectroscopic observations of emission lines in the far-infrared, where some of the most important gas coolants emit, such as the [OI] ^3^P_1_-^3^P_2_ transition at 63.18 microns. We provide a compilation of observations of far-IR lines in 362 young stellar objects covering all evolutionary stages, from Class 0 to Class III with debris discs. In the present paper we focus on [OI] and o-H_2_O emission at 63 microns. We have retrieved all the available Herschel-PACS spectroscopic observations at 63 microns that used the dominant observing mode, the chop-nod technique. We provide measurements of line fluxes for the [OI] ^3^P_1_-^3^P_2_ and o-H_2_O 8_08_-7_17_ transitions at 63 microns computed using different methods. Taking advantage of the PACS IFU, we check for spatially extended emission and further study the presence of multiple dynamical components in line emission. The final compilation consists of line and continuum fluxes at 63 microns for a total of 362 young stellar objects (YSOs). We detected [OI] line emission at 63 microns in 194 sources out of 362, and line absorption in another five sources. o-H_2_O was detected in 42 sources. We find evidence of extended [OI] emission in 77 sources, and detect 3sigma residual emission in 71 of them. The number of sources showing extended emission decays from Class 0 to Class II. We also looked for different components contributing to the line emission, and found evidence for multiple components in 30 sources. We explored correlations between line emission and continuum emission and find a clear correlation between WISE fluxes from 4.6 to 22 microns and [OI] line emission. We conclude that the observed emission is typically a combination of disc/envelope and jet emission.2016A&A...594A..59Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/594/A59CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/594/A59https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/594/A59http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/594/A59https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/594/A59https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/594/A59http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/594/A59GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/594/A59/tableb1 (description, including name, position, spectral type, source class and cluster)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/594/A59/tableb1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/594/A59/tableb1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/594/A59/tableb1?GETtext/xml+votable180.050000true1.468958-41.7530670.005555555555555556Cone search capability for table J/A+A/594/A59/tableb2 (Line and continuum fluxes from central spaxel)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/594/A59/tableb2?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/594/A59/tableb2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/594/A59/tableb2?GETtext/xml+votable180.050000true1.468958-41.7530.0055555555555555565/270 292 6/342 489 857-860 862 881 1029 1031 1039-1040 1043 1048 1050-1054 1061 1063 1073-1075 1111 1113-1115 1123-1124 1136 1154 1156 1159 1539 1606 3649 6495 14317 14689 14704 14906 15422 15426 15630 15683 15965 16132 17421 17425 17887 18203 18205 19509 19598 20125 20831 21023 21080 21083 21289 21430 21480 22023 22416 22873 22876 23376 23533 23548-23549 23551 23593 23636 23704 24203 24277 24279 24281 24300 24449 24629 25113 28762 28921 29101 29193 29207 29653 30318 30341 30343 30352 30366 30519 30613 30733 30821 31078 31259 31537 31629 31640 31642 31653 31664 31765 32065 32083 33694 34054 34823 34993 35497 36130 36697 36948 36956-36957 37012-37013 37128 37186 37978 38002 38347 38363 38382 38687 38742 39248 39735 39753 41126-41127 41132 41134 41472 41812 42233 42456 42595 42605 42610-42611 42614 42644 42704-42705 42736 42885 42911 42931 42970 42972 42981 42983 42990-42992 42994 43010 43029 43175 43670 43677 44049 44069 44311 44317 44319 44321 44361-44362 44366-44367 44378-44379 44389 44401 45746 46939 47205 47464 47626 47742 47826 47828 48274 48651https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/594/A59?format=asciiInfrareddefaultJ/A+A/594/A59/tableb1description, including name, position, spectral type, source class and clusterSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource name (G2)meta.id;meta.maincharRAJ2000Source right ascension (J2000.0)degpos.eq.ra;meta.mainDEJ2000Source declination (J2000.0)degpos.eq.dec;meta.mainSpTypeSource spectral typesrc.spTypecharDiscTypeSource classificationsrc.classcharAssocSource association, if anymeta.id.parentcharJ/A+A/594/A59/tableb2Line and continuum fluxes from central spaxelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource name (G2)meta.id;meta.maincharRAJ2000Source right ascension (J2000.0) (G2)degpos.eq.ra;meta.mainDEJ2000Source declination (J2000.0) (G2)degpos.eq.dec;meta.mainOBSIDHerschel OBSID for this observationmeta.id;obsFOIOI line flux at 63.185 microns1e-18W.m**-2phot.flux;em.IR.60-100um;spect.lineinte_FOI? OI line flux error at 63.185 microns (an error of 0.0 is given for upper limits)1e-18W.m**-2stat.errorintnullablel_FOI[0/1] Limit flag on OI line flux (G1)meta.code.errorcharFH2Oo-H2O line flux at 63.323 microns1e-18W.m**-2phot.flux;em.IR.60-100um;spect.lineinte_FH2O? o-H2O line flux error at 63.323 microns (an error of 0.0 is given for upper limits)1e-18W.m**-2stat.errorintnullablel_FH2O[0/1] Limit flag on o-H2O line flux (G1)meta.code.errorcharF63Continuum flux at 63 micronsJyphot.flux.density;em.IR.30-60umdoublee_F63? Error in continuum flux at 63 microns (an error of 0.0 is given for upper limits)Jystat.errorfloatnullablel_F63[0/1] Limit flag on continuum at 63 microns flux (G1)meta.code.errorcharJ/A+A/594/A59/tableb3[OI] line flux from central spaxel, central 3x3 spaxel and integrated IFUrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource namemeta.id;meta.maincharOBSIDHerschel OBSID for this observationmeta.id;obsFOIOI line flux at 63.185 microns1e-18W.m**-2phot.flux;em.IR.60-100um;spect.lineinte_FOI? OI line flux error at 63.185 microns (an error of 0.0 is given for upper limits)1e-18W.m**-2stat.errorintnullablel_FOI[0/1] Limit flag on OI line flux (G1)meta.code.errorcharFOI3x3OI line flux at 63.185 microns from co-adding the central 3x3 spaxel1e-18W.m**-2phot.flux;em.IR.60-100um;spect.lineinte_FOI3x3? OI line flux error at 63.185 microns from co-adding the central 3x3 spaxel (an error of 0.0 is given for upper limits)1e-18W.m**-2stat.errorintnullablel_FOI3x3[0/1] Limit flag on OI line flux from central 3x3 spaxel (G1)meta.code.errorcharFOI5x5OI line flux at 63.185 microns from co-adding 5x5 spaxel in the IFU1e-18W.m**-2phot.flux;em.IR.60-100um;spect.lineinte_FOI5x5? OI line flux error at 63.185 microns from co-adding 5x5 spaxel in the IFU (an error of 0.0 is given for upper limits)1e-18W.m**-2stat.errorintnullablel_FOI5x5[0/1] Limit flag on OI line flux from co-adding 5x5 spaxel in the IFU (G1)meta.code.errorchar