Degirmenci, OLSezer, CDemircan, OErdem, AOzdemir, SAk, HAlbayrak, B2019-10-272019-10-2719990365-01380365-0138https://hdl.handle.net/11454/34464New 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.eninfo:eu-repo/semantics/openAccessstars : binaries : eclipsingstars : individual : V 382 CygArticle1342327331WOS:000078294400013N/AQ2