Variable Stars in the LMC Globular Cluster NGC 1754

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dc.catalogadorpau
dc.contributor.authorKuehn, Charles A., III
dc.contributor.authorTaylor, L.
dc.contributor.authorSmith, H. A.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorPritzl, B. J.
dc.contributor.authorDe Lee, N.
dc.date.accessioned2024-03-05T15:15:08Z
dc.date.available2024-03-05T15:15:08Z
dc.date.issued2006
dc.description.abstractWe have used BVI observations taken with the SMARTS 1.3m telescope and with the SOAR telescope to identify variable stars in the vicinity of the old LMC cluster NGC 1754. We present light curves and periods for the variables and classify the variables according to type. The probability that the RR Lyrae stars found in the neighborhood of NGC 1754 actually belong to the cluster is discussed. Unlike most globular clusters of the Milky Way halo, many of the old star clusters of the LMC have Oosterhoff intermediate properties. The Oosterhoff classification of field and cluster RR Lyrae stars near NGC 1754 is considered. We thank the NSF for partial support of this research....
dc.fuente.origenORCID
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/2006AAS...209.2907K/abstract
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84116
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsacceso restringido
dc.titleVariable Stars in the LMC Globular Cluster NGC 1754
dc.typecomunicación de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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