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dc.contributor.authorOzkan, Mustafa Türker
dc.contributor.authorPlevne, Olcay
dc.contributor.authorCoskunoglu, Başar
dc.date.accessioned2021-03-05T07:30:42Z
dc.date.available2021-03-05T07:30:42Z
dc.date.issued2019
dc.identifier.citationCoskunoglu B., Plevne O., Ozkan M. T. , "Gould Belt members in X-ray RAVE: cross-matching RAVE stars with 3XMM point sources", ASTROPHYSICS AND SPACE SCIENCE, cilt.364, 2019
dc.identifier.issn0004-640X
dc.identifier.otherav_9426701a-0d67-4271-a6ea-b6153e5f07d3
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/99810
dc.identifier.urihttps://doi.org/10.1007/s10509-019-3505-4
dc.description.abstractIn this paper the results of matching the RAdial Velocity Experiment (RAVE), a spectroscopic Southern hemisphere survey (9<IDENIS<12), and XMM-Newton Serendipitous Source Catalogue (3XMM) are presented. The latest data releases of RAVE and XMM were matched and a X-ray RAVE catalogue of 1071 stars was obtained. Then the catalogue was checked for possible Gould Belt (GB) members. We obtained a subsample of 10 stars that meet the GB membership criteria. This subsample and GB member candidates were tested photometrically and kinematically. Among the members there are two BY Dra type variables, an NGC2451 open cluster member, a high proper motion star. The rest are regular main sequence stars. The members have very low velocity dispersions which lead us to think that the members belong in a single structure. We also found out that a kinematical GB membership test might be possible to derive given a large enough GB member sample as they fit in a narrow interval in space velocity diagrams.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleGould Belt members in X-ray RAVE: cross-matching RAVE stars with 3XMM point sources
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume364
dc.identifier.issue1
dc.contributor.firstauthorID260205


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