Multicolor Photometric Behavior of the Young Stellar Object V1704 Cygni

dc.contributor.author Ibryamov, Sunay
dc.contributor.author Semkov, Evgeni
dc.contributor.author Peneva, Stoyanka
dc.contributor.author Karadeniz, Uğur
dc.date.accessioned 2020-07-25T22:09:21Z
dc.date.available 2020-07-25T22:09:21Z
dc.date.issued 2018
dc.description.abstract Results from BV RI photometric observations of the pre-main sequence star V1704 Cyg collected during the time period from August 2010 to December 2017 are presented. The star is located in the star-forming HII region IC 5070 and it exhibits photometric variability in all optical passbands. After analyzing the obtained data, V1704 Cyg is classified as a classical T Tauri star. en_US
dc.identifier.issn 1313-2709
dc.identifier.issn 1314-5592
dc.identifier.scopus 2-s2.0-85065654665
dc.identifier.uri https://hdl.handle.net/11147/9288
dc.language.iso en en_US
dc.publisher Bulgarian Acad Sciences, Inst Astronomy en_US
dc.relation.ispartof Bulgarian Astronomical Journal en_US
dc.rights info:eu-repo/semantics/openAccess en_US
dc.subject Stars: pre-main sequence en_US
dc.subject Stars: variables: T Tauri en_US
dc.subject Star: individual: (V1704 Cyg) en_US
dc.title Multicolor Photometric Behavior of the Young Stellar Object V1704 Cygni en_US
dc.type Article en_US
dspace.entity.type Publication
gdc.author.institutional Karadeniz, Uğur
gdc.coar.access open access
gdc.coar.type text::journal::journal article
gdc.description.department İzmir Institute of Technology. Physics en_US
gdc.description.endpage 18 en_US
gdc.description.publicationcategory Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı en_US
gdc.description.scopusquality Q4
gdc.description.startpage 10 en_US
gdc.description.volume 29 en_US
gdc.description.wosquality Q4
gdc.identifier.wos WOS:000438559700002
gdc.index.type WoS
gdc.index.type Scopus
gdc.scopus.citedcount 0
gdc.wos.citedcount 0
relation.isOrgUnitOfPublication.latestForDiscovery 9af2b05f-28ac-4003-8abe-a4dfe192da5e

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