Period Changes of Two Contact Binaries: DF Hya and WZ And
dc.contributor.author | Bulut, A. | |
dc.contributor.author | Bulut, I. | |
dc.date.accessioned | 2025-01-27T21:07:14Z | |
dc.date.available | 2025-01-27T21:07:14Z | |
dc.date.issued | 2018 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description | 33rd International Physics Congress of the Turkish-Physical-Society (TPS) -- SEP 06-10, 2017 -- Bodrum, TURKEY | |
dc.description.abstract | Orbital period variations of two contact binaries DF Hya and WZ And are analyzed with the least-squares method by using all available minima times. It is shown that the period variations of these systems are due mainly to the LightTime Effect (LITE) due originates from gravitational influence of a third body. New LITE elements such as, orbital periods and minimum masses of possibility third bodies are given. | |
dc.description.sponsorship | Turkish Phys Soc | |
dc.identifier.doi | 10.1063/1.5026003 | |
dc.identifier.isbn | 978-0-7354-1627-7 | |
dc.identifier.issn | 0094-243X | |
dc.identifier.scopus | 2-s2.0-85043986490 | |
dc.identifier.scopusquality | Q4 | |
dc.identifier.uri | https://doi.org/10.1063/1.5026003 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/27941 | |
dc.identifier.volume | 1935 | |
dc.identifier.wos | WOS:000445956100049 | |
dc.identifier.wosquality | N/A | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.publisher | Amer Inst Physics | |
dc.relation.ispartof | Turkish Physical Society 33rd International Physics Congress (Tps33) | |
dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | binaries | |
dc.subject | eclipsing | |
dc.subject | ligh-time effect | |
dc.subject | stars: individual DF Hya and WZ And | |
dc.title | Period Changes of Two Contact Binaries: DF Hya and WZ And | |
dc.type | Conference Object |