A Search for EHB Pulsators in the Globular Cluster NGC 6752

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dc.catalogadorkjc
dc.contributor.authorCatelan , Marcio
dc.contributor.authorPrieto, G. E.
dc.contributor.authorZoccali, M.
dc.contributor.authorWeidner, C.
dc.contributor.authorStetson, P. B.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorAltmann, M.
dc.contributor.authorSmith, H. A.
dc.contributor.authorPritzl, B. J.
dc.contributor.authorBorissova, J.
dc.contributor.authorde Medeiros, J. R.
dc.date.accessioned2024-03-04T17:01:54Z
dc.date.available2024-03-04T17:01:54Z
dc.date.issued2007
dc.description.abstractWe describe the status of a project whose main goal is to detect variability along the extreme horizontal branch of the globular cluster NGC 6752. Based on Magellan 6.5-m data, preliminary light curves are presented for some candidate variables. By combining our time-series data, we also produce a deep CMD of unprecedented quality for the cluster which reveals a remarkable lack of main sequence binaries, possibly pointing to a low primordial binary fraction....
dc.fuente.origenORCID
dc.identifier.urihttps://arxiv.org/pdf/0710.0600.pdf
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/83758
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsacceso abierto
dc.titleA Search for EHB Pulsators in the Globular Cluster NGC 6752
dc.typecomunicación de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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