C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud : analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibrium

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dc.contributor.authorRoueff, A.
dc.contributor.authorGerin, M.
dc.contributor.authorGratier, P.
dc.contributor.authorLevrier, F.
dc.contributor.authorPety, J.
dc.contributor.authorGaudel, M.
dc.contributor.authorGoicoechea, J. R.
dc.contributor.authorOrkisz, J. H.
dc.contributor.authorDe Souza Magalhaes, V.
dc.contributor.authorGuzmán Veloso, Viviana Gabriela
dc.contributor.authorVono, M.
dc.contributor.authorBardeau, S.
dc.contributor.authorBron, E.
dc.contributor.authorChanussot, J.
dc.contributor.authorChainais, P.
dc.contributor.authorHughes, A.
dc.contributor.authorKainulainen, J.
dc.contributor.authorLanguignon, D.
dc.contributor.authorLe Bourlot, J.
dc.contributor.authorLe Petit, F.
dc.contributor.authorLiszt, H. S.
dc.contributor.authorMarchal, A.
dc.contributor.authorMiville Deschênes, M. A.
dc.contributor.authorPeretto, N.
dc.contributor.authorRoueff, E.
dc.contributor.authorSievers, A.
dc.date.accessioned2021-06-22T22:50:39Z
dc.date.available2021-06-22T22:50:39Z
dc.date.issued2021
dc.fechaingreso.objetodigital2024-07-16
dc.format.extent27 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1051/0004-6361/202037776
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.scopusid2-s2.0-85098574061
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202037776
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/60799
dc.identifier.wosidWOS:000603602100002
dc.information.autorucInstituto de Física ; Guzmán Veloso, Viviana Gabriela ; 0000-0003-4784-3040 ; 1083356
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final27
dc.pagina.inicio1
dc.revistaAstronomy and Astrophysicses_ES
dc.rightsacceso abierto
dc.titleC18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud : analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibriumes_ES
dc.typeartículo
dc.volumenVol. 645
sipa.codpersvinculados1083356
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