Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7315
Full metadata record
DC FieldValueLanguage
dc.contributor.authorDar, A. A-
dc.contributor.authorParihar, P. S-
dc.contributor.authorSaleh, P-
dc.contributor.authorMalik, M. A-
dc.date.accessioned2018-07-11T06:06:46Z-
dc.date.available2018-07-11T06:06:46Z-
dc.date.issued2018-10-
dc.identifier.citationNew Astronomy, Vol. 64, pp. 34-39en_US
dc.identifier.issn1384-1076-
dc.identifier.urihttp://hdl.handle.net/2248/7315-
dc.descriptionRestricted Accessen_US
dc.description.abstractThis work presents the first photometric variability survey of the open cluster NGC 2509 carried out in February, 2017. Data of four nights was analysed by ensemble photometry technique, using 1k × 1k CCD and 1.3 m telescope in V and B filters. The observations were carried out upto limiting magnitude (v∼20) in both V and B filters to search for variable stars. From the phase plots using periods obtained from Schuster and Lomb Scargle periodogram, 16 objects were classified as suspected variables owing to their low amplitude variations in phase. For the remaining objects in the cluster, it is hard to establish their variability.en_US
dc.language.isoenen_US
dc.publisherElsevier B.Ven_US
dc.relation.urihttps://doi.org/10.1016/j.newast.2018.04.002-
dc.rights© Elsevier B.V-
dc.subjectVariable starsen_US
dc.subjectPhotometryen_US
dc.subjectPeriodogramen_US
dc.subjectNGC 2509en_US
dc.titleSearch for variable stars in the open cluster NGC 2509en_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Search for variable stars in the open cluster NGC 2509.pdfRestricted Access1.22 MBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.