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hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorBRON, E.
dc.contributor.authorDAUDON, C.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorPETY, J.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorLEVRIER, F.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorGERIN, M.
hal.structure.identifierAMOR 2017
dc.contributor.authorGRATIER, P.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorORKISZ, Jan
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorGUZMÁN, V.
hal.structure.identifierServices communs OMP [UMS 831]
dc.contributor.authorBARDEAU, S.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorGOICOECHEA, J. R.
dc.contributor.authorLISZT, H.
dc.contributor.authorOEBERG, K.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorPERETTO, N.
hal.structure.identifierInstituto de RadioAstronomía Milimétrica [IRAM]
dc.contributor.authorSIEVERS, A.
hal.structure.identifierUniversity of Exeter
dc.contributor.authorTREMBLIN, Pascal
dc.date.issued2017
dc.descriptionVizieR On-line Data Catalog: J/A+A/610/A12. Originally published in: 2018A&A...610A..12B
dc.description.abstractEnIntegrated line intensities maps (in the 9-12km/s range) of the Orion B molecular cloud in $^{12}$CO(1-0), $^{13}$CO(1-0), C$^{18}$O(1-0), CN(1-0), HCO$^+$(1-0), used as basis for the clustering analysis presented in the paper. Maps of the cluster attributions of each pixel resulting from the two clustering analyses presented (based on CO isotopes only, and based on CO isotopes, HCO$^+$ and CN) are also included. Description of the fits files: - ClustCO.fit : Cluster assignation map from the clustering analysis based on CO isotopes only. - ClustFUV.fit : Cluster assignation map from the clustering analysis based on CO isotopes, HCO+ and CN. - map$^{12}$CO.fit : Integrated intensity (9-12km/s) map of the $^{12}$CO J=1-0 line. - map$^{13}$CO.fit : Integrated intensity (9-12km/s) map of the $^{13}$CO J=1-0 line. - mapC$^{18}$O.fit : Integrated intensity (9-12km/s) map of the C$^{18}$O J=1-0 line. - mapCN.fit : Integrated intensity (9-12km/s) map of the CN N=1-0 line. - mapHCOp.fit : Integrated intensity (9-12km/s) map of the HCO$^+$ J=1-0 line. (2 data files).
dc.language.isoen
dc.subject.enMolecular clouds
dc.subject.enInterstellar medium
dc.subject.enSpectrophotometry
dc.subject.enCarbon monoxide
dc.title.enVizieR Online Data Catalog: Clustering the Orion B giant molecular cloud (Bron+, 2018)
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
hal.identifierhal-01725083
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01725083v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2017&rft.au=BRON,%20E.&DAUDON,%20C.&PETY,%20J.&LEVRIER,%20F.&GERIN,%20M.&rft.genre=unknown


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