{"title":"对流不稳定导致的前行星盘的偶发性吸积","authors":"L. Maksimova, Y. Pavlyuchenkov","doi":"10.15826/b978-5-7996-2935-9.59","DOIUrl":null,"url":null,"abstract":"Using the model of viscous evolution of the disk and the calculation of the vertical structure, the evolution of the Keplerian disk and its morphology are investigated. The episodic nature of accretion was revealed and the effect of various initial parameters on the behavior of flashes in the protoplanetary disk was investigated.","PeriodicalId":183711,"journal":{"name":"Proceedings of the 48-th International student's conferences \"Physics of Space\"","volume":"70 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"EPISODIC ACCRETION IN PROPLANETARY DISCS AS A RESULT OF CONVECTIVE INSTABILITY\",\"authors\":\"L. Maksimova, Y. Pavlyuchenkov\",\"doi\":\"10.15826/b978-5-7996-2935-9.59\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Using the model of viscous evolution of the disk and the calculation of the vertical structure, the evolution of the Keplerian disk and its morphology are investigated. The episodic nature of accretion was revealed and the effect of various initial parameters on the behavior of flashes in the protoplanetary disk was investigated.\",\"PeriodicalId\":183711,\"journal\":{\"name\":\"Proceedings of the 48-th International student's conferences \\\"Physics of Space\\\"\",\"volume\":\"70 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of the 48-th International student's conferences \\\"Physics of Space\\\"\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.15826/b978-5-7996-2935-9.59\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of the 48-th International student's conferences \"Physics of Space\"","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.15826/b978-5-7996-2935-9.59","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
EPISODIC ACCRETION IN PROPLANETARY DISCS AS A RESULT OF CONVECTIVE INSTABILITY
Using the model of viscous evolution of the disk and the calculation of the vertical structure, the evolution of the Keplerian disk and its morphology are investigated. The episodic nature of accretion was revealed and the effect of various initial parameters on the behavior of flashes in the protoplanetary disk was investigated.