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hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorGOICOECHEA, J. R.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorPETY, J.
dc.contributor.authorCHAPILLON, E.
hal.structure.identifierCentro de Astrobiologia [Madrid] [CAB]
dc.contributor.authorCERNICHARO, J.
hal.structure.identifierLaboratoire de Radioastronomie [LRA]
dc.contributor.authorGERIN, M.
hal.structure.identifierDepartamento de Ingenieria Eléctrica [DIE]
dc.contributor.authorHERRERA, C.
dc.contributor.authorREQUENA-TORRES, M. A.
dc.contributor.authorSANTA-MARIA, M. G.
dc.date.issued2018
dc.descriptionVizieR On-line Data Catalog: J/A+A/618/A35. Originally published in: 2018A&A...618A..35G
dc.description.abstractEnThe FITS files contain total integrated line intensity maps of CO (3-2), H13CN (4-3) and SO (89-78) emission lines shown in Figures 1, 3, 4 and A4 and A4 of the article. The integrated velocity range goes from vLSR=-150 to +150km/s for H13CN and SO and from -400 to +280 for CO. The intensity scale of the images is in K.km/s units. (2 data files).
dc.language.isoen
dc.subject.enInterstellar medium
dc.subject.enMolecular clouds
dc.subject.enInterferometry
dc.title.enVizieR Online Data Catalog: ALMA images of the CND and SgrA* (Goicoechea+, 2018)
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
hal.identifierhal-01901682
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01901682v1
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