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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7327
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dc.contributor.authorArellano Ferro, A-
dc.contributor.authorBramich, D. M-
dc.contributor.authorGiridhar, S-
dc.contributor.authorLuna, A-
dc.contributor.authorMuneer, S-
dc.date.accessioned2020-11-20T13:27:28Z-
dc.date.available2020-11-20T13:27:28Z-
dc.date.issued2015-04-
dc.identifier.citationInformation Bulletin on Variable Stars, No. 6137en_US
dc.identifier.issn0374-0676-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7327-
dc.descriptionOpen Access © Konkoly Observatory http://ibvs.konkoly.hu/cgi-bin/IBVSpdf?6137en_US
dc.description.abstractWe report twelve variables not previously detected in the globular cluster M5 (NGC 5904); one SX Phe and eleven semi-regular variables (SR). Their identifications, equatorial coordinates, ephemerides, and light curves are given. Furthermore, we have explored the light curves of a group of stars whose variability has not been confirmed and that are marked as probable non- variables in the CVSGC. Finally, we offer detailed identifications for some of the known variables in crowded regions that were misidentified in previous studies. We shall also address the cases of the cataclysmic variable or U Gem type V101 and of the variable blue straggler V159.en_US
dc.language.isoenen_US
dc.publisherKonkoly Observatoryen_US
dc.subjectAstrophysics - Solar and Stellar Astrophysicsen_US
dc.titleNew variables in M5 (NGC 5904) and some identification correctionsen_US
dc.typeArticleen_US
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