Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7892
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dc.contributor.authorYepez, M. A-
dc.contributor.authorFerro, A. Arellano-
dc.contributor.authorSchröder, K. P.-
dc.contributor.authorMuneer, S-
dc.contributor.authorGiridhar, Sunetra-
dc.contributor.authorAllen, Christine-
dc.date.accessioned2021-12-29T05:29:42Z-
dc.date.available2021-12-29T05:29:42Z-
dc.date.issued2021-06-
dc.identifier.citationASP Conference Series, Vol. 529, pp. 184-188en_US
dc.identifier.urihttp://hdl.handle.net/2248/7892-
dc.descriptionRestricted accessen_US
dc.description.abstractWe present new CCD VI photometry of the globular cluster Pal 13. Fourier decomposition of the light curves of RRab stars lead to estimations of [Fe/H]ZW = -1.65±0.15, and a distance to the cluster of 23.67±0.57 kpc. A colour-magnitude diagram, built exclusively with likely star members, shows consistency with the above parameters and an age of 12 Gyrs. A search of variable stars in the field of view of our images revealed the variability of a red giant cluster member and of three probably non-member stars: two RRab and one BL Her star. The Gaia-DR2 proper motions of member stars in Pal 13 show a significant scatter, consistent with the scenario of the cluster being tidally stripped.en_US
dc.language.isoenen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.relation.urihttp://www.aspbooks.org/a/volumes/article_details/?paper_id=39997-
dc.rights© Astronomical Society of the Pacific-
dc.titleVariable Stars in Palomar 13; an Evaporating Globular Clusteren_US
dc.typeArticleen_US
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