OBSERVATIONAL DATA FOR THE KINEMATICS OF THE LOCAL UNIVERSE .1. RADIAL-VELOCITY MEASUREMENTS

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dc.contributor.authorBOTTINELLI, L
dc.contributor.authorDURAND, N
dc.contributor.authorFOUQUE, P
dc.contributor.authorGARNIER, R
dc.contributor.authorGOUGUENHEIM, L
dc.contributor.authorPATUREL, G
dc.contributor.authorTEERIKORPI, P
dc.date.accessioned2025-01-23T19:22:14Z
dc.date.available2025-01-23T19:22:14Z
dc.date.issued1992
dc.description.abstractThe study of the local velocity field requires the use of a very large sample to describe as accurately as possible some prominent features of the local kinematics. The problem of collecting a large sample is made more difficult because of the Malmquist bias which plagues distance determinations. Our programme aims at determining bias-free distances for a complete sample in order to study the local velocity field. The present paper gives 303 preliminary optical and radio redshifts measured for this program at ESO, OHP and Nancay Observatories.
dc.fuente.origenWOS
dc.identifier.issn0365-0138
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/98997
dc.identifier.wosidWOS:A1992HL04100008
dc.issue.numero1
dc.language.isoen
dc.pagina.final188
dc.pagina.inicio173
dc.revistaAstronomy & astrophysics supplement series
dc.rightsacceso restringido
dc.subjectCATALOGS
dc.subjectGALAXIES DISTANCES AND REDSHIFT
dc.subjectRADIO LINES ATOMIC
dc.titleOBSERVATIONAL DATA FOR THE KINEMATICS OF THE LOCAL UNIVERSE .1. RADIAL-VELOCITY MEASUREMENTS
dc.typeartículo
dc.volumen93
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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