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dc.contributor.authorHernandez-Toledo, H.M.en_US
dc.contributor.authorHuchtmeier, W.en_US
dc.contributor.authorKarachentseva, V.E.en_US
dc.contributor.authorBrinks, E.en_US
dc.date.accessioned2008-01-30T10:45:14Z
dc.date.available2008-01-30T10:45:14Z
dc.date.issued2002en_US
dc.identifier.citationIn: Procs of Disks of Galaxies: Kinematics, Dynamics and Perturbations - ASP Conf Series 275 p.449en_US
dc.identifier.isbn1-58381-117-6en
dc.identifier.other901612en_US
dc.identifier.urihttp://hdl.handle.net/2299/1485
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/253.html--Copyright Astronomical Society of the Pacificen
dc.description.abstractWe present preliminary results from Effelsberg 100-m HI observations of a sample of 27 Triple Galaxies selected from the Karachentseva Catalogue of Isolated Triplets. These observations were complemented with optical CCD BVRIHa images taken at Observatorio Astronomico Nacional, San Pedro Martir, Mexico. Our results confirm that a significant fraction of the observed sample are physically associated.en
dc.format.extent74547 bytes
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.titleHI Observations of Isolated Triple Galaxies.en_US
dc.typeConference paperen_US
herts.preservation.rarelyaccessedtrue


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