The First Photometric Study of W UMa Binary System V1833 Ori
dc.authorid | TANRIVER, Mehmet/0000-0002-3263-9680 | |
dc.contributor.author | Tanrıver, Mehmet | |
dc.contributor.author | Bulut, Ahmet | |
dc.date.accessioned | 2025-01-27T20:39:17Z | |
dc.date.available | 2025-01-27T20:39:17Z | |
dc.date.issued | 2022 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description.abstract | The first photometric solution in the B, V, R-c and I-c filters of the short period V1833 Ori eclipsing binary is presented based on new ground-based CCD photometric observations. We analyzed the BVRI photometric light curves of the system, using PHOEBE 0.31a, a binary star modeling program, with the Wilson-Devinney method based on Roche geometry to achieve the best accordance with the photometric observations to determine their absolute parameters from the light curves. We updated the ephemeris of V1833 Ori using two new light curve minima derived by our new observational data from those collected in the literature and analyzed the change of the system's orbital period. The O-C analysis indicates that the variations of the orbital period of V1833 Ori with time are increasing at a rate of 3.03 x 10(-7) days yr(-1). The distance of V1833 Ori is 173.7 +/- 15.6 pc. From the solutions, we find that V1833 Ori is an A-subtype W UMa overcontact binary with q = 0.701 mass ratio and f = 1.14 fill-out factor. The HR diagram positions of the eclipsing binary system's components are discussed. The system's absolute dimensions were compared to those of similar binaries in the log T-eff - log L, logM - logL, logM - logR and log M - log J(0) diagrams. | |
dc.description.sponsorship | Scientific Research Projects Coordination Unit of Erciyes University [FBA-09-788] | |
dc.description.sponsorship | This study was supported by the Scientific Research Projects Coordination Unit of Erciyes University (project number FBA-09-788). We thank Canakkale Onsekiz Mart University Ulupnar Observatory (COMU-UPO) for support in allowing use of their T30 telescope. We gratefully acknowledge the SIMBAD, ADS, CRTS, TESS, BRNO O-C Gateway, Krakow O-C Atlas and NASA/IPAC databases for also providing data. We acknowledge with thanks the variable star observations from the AAVSO International Database contributed by observers worldwide and used in this research. We are also grateful to the referees, the editors and everyone involved who provided constructive suggestions and comments for this article. | |
dc.identifier.doi | 10.1088/1674-4527/ac7af7 | |
dc.identifier.issn | 1674-4527 | |
dc.identifier.issn | 2397-6209 | |
dc.identifier.issue | 8 | |
dc.identifier.scopus | 2-s2.0-85136106610 | |
dc.identifier.scopusquality | Q2 | |
dc.identifier.uri | https://doi.org/10.1088/1674-4527/ac7af7 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/23910 | |
dc.identifier.volume | 22 | |
dc.identifier.wos | WOS:000832756800001 | |
dc.identifier.wosquality | Q3 | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.publisher | Natl Astronomical Observatories, Chin Acad Sciences | |
dc.relation.ispartof | Research in Astronomy and Astrophysics | |
dc.relation.publicationcategory | info:eu-repo/semantics/openAccess | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | (stars:) binaries: eclipsing | |
dc.subject | stars: fundamental parameters | |
dc.subject | stars: individual (V1833 Ori) | |
dc.title | The First Photometric Study of W UMa Binary System V1833 Ori | |
dc.type | Article |