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Authordc.contributor.authorGaray Brignardello, Guido es_CL
Authordc.contributor.authorRodríguez, Luis F. es_CL
Authordc.contributor.authorDe Gregorio Monsalvo, Itziar es_CL
Admission datedc.date.accessioned2008-05-14T14:08:56Z
Available datedc.date.available2008-05-14T14:08:56Z
Publication datedc.date.issued2007es_CL
Cita de ítemdc.identifier.citationASTRONOMICAL JOURNAL Vol. 134 SEP 2007 3 906-911es_CL
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/124711
General notedc.descriptionPublicación ISIes_CL
Abstractdc.description.abstractWe present radio-continuum observations at 7 mm made using the Very Large Array toward three massive star-forming regions thought to be in very early stages of evolution, selected from the 2002 sample of Sridharan et al. Emission was detected toward all three sources ( IRAS 18470-0044, IRAS 19217+1651, and IRAS 23151+5912). We find that in all cases the 7 mm emission corresponds to thermal emission from ionized gas. The regions of ionized gas associated with IRAS 19217+1651 and IRAS 23151+5912 are hypercompact, with diameters of 0.009 and 0.0006 pc and emission measures of 7.0 x 10(8) and 2.3 x 10(9) pc cm(-6), respectively.es_CL
Lenguagedc.language.isoenes_CL
Keywordsdc.subjectH (II) regionses_CL
Area Temáticadc.subject.otherAstronomy & Astrophysicses_CL
Títulodc.titleVery large array observations of candidate high-mass protostellar objects at 7 millimeterses_CL
Document typedc.typeArtículo de revista


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