The early type contact binary system V 382 Cygni
| dc.contributor.author | Degirmenci, ÖL | |
| dc.contributor.author | Sezer, C | |
| dc.contributor.author | Demircan, O | |
| dc.contributor.author | Erdem, A | |
| dc.contributor.author | Özdemir, S | |
| dc.contributor.author | Ak, H | |
| dc.contributor.author | Albayrak, B | |
| dc.date.accessioned | 2025-01-27T20:27:04Z | |
| dc.date.available | 2025-01-27T20:27:04Z | |
| dc.date.issued | 1999 | |
| dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
| dc.description.abstract | New photometric data set of the early type contact binary V382 Cyg have been analyzed with emphasis on determining the photometric mass ratio of the system. The result (q = 0.68) supports the value given by Popper & Hill (1991). A study of the system using new data shows a period increase of about 3.28 s per century, which corresponds to a very large rate similar to 5.0 10(-6) M./yr of mass transfer from the less massive to the more massive component under the conservative mass transfer hypothesis. | |
| dc.identifier.endpage | 331 | |
| dc.identifier.issn | 0365-0138 | |
| dc.identifier.issue | 2 | |
| dc.identifier.scopus | 2-s2.0-4243230007 | |
| dc.identifier.scopusquality | N/A | |
| dc.identifier.startpage | 327 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12428/22570 | |
| dc.identifier.volume | 134 | |
| dc.identifier.wos | WOS:000078294400013 | |
| dc.identifier.wosquality | Q2 | |
| dc.indekslendigikaynak | Web of Science | |
| dc.indekslendigikaynak | Scopus | |
| dc.language.iso | en | |
| dc.publisher | E D P Sciences | |
| dc.relation.ispartof | Astronomy & Astrophysics Supplement Series | |
| dc.relation.publicationcategory | info:eu-repo/semantics/openAccess | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.snmz | KA_WoS_20250125 | |
| dc.subject | stars : binaries : eclipsing | |
| dc.subject | stars : individual : V 382 Cyg | |
| dc.title | The early type contact binary system V 382 Cygni | |
| dc.type | Article |
