VLBA Determination of the Distance to Nearby Star‐forming Regions. I. The Distance to T Tauri with 0.4% Accuracy

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dc.contributor.authorLoinard, Laurent
dc.contributor.authorLachaume, Regis
dc.contributor.authorTorres, Rosa M.
dc.contributor.authorMioduszewski, Amy J.
dc.contributor.authorRodríguez J., Luis F.
dc.contributor.authorGonzález-Lópezlira, Rosa A.
dc.contributor.authorVázquez, Virgilio
dc.contributor.authorGonzález, Erandy
dc.date.accessioned2019-05-23T15:37:58Z
dc.date.available2019-05-23T15:37:58Z
dc.date.issued2007
dc.date.updated2019-05-16T19:15:44Z
dc.fuente.origenORCID
dc.identifier.doi10.1086/522493
dc.identifier.issn1538-4357
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/22546
dc.issue.numeroNo. 1
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final554
dc.pagina.inicio546
dc.relation.isformatofThe Astrophysical Journal, vol. 671, no. 1 (dec. 2007), pp. 546-554.
dc.revistaThe Astrophysical Journales_ES
dc.rightsacceso abierto
dc.subjectAstrometryes_ES
dc.subjectbinaries generales_ES
dc.subjectMagnetic fieldses_ES
dc.subjectRadiation mechanisms nonthermales_ES
dc.subjectRadio continuum starses_ES
dc.subjectStars formationes_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleVLBA Determination of the Distance to Nearby Star‐forming Regions. I. The Distance to T Tauri with 0.4% Accuracyes_ES
dc.typeartículo
dc.volumenVol. 671
sipa.codpersvinculados1008654
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