{"title":"新的不透明对磁盘不稳定性的影响","authors":"M. Takeuti, R. Kanetake","doi":"10.1063/1.45938","DOIUrl":null,"url":null,"abstract":"The vertical oscillation of an accretion disk surrounding a neutron star is studied by using the OPAL opacities. We have found that the vertical structure of the model disk is vibrationally unstable when we use new opacities instead of the Los Alamos opacities.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"118 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Effect of new opacities on the disk instability\",\"authors\":\"M. Takeuti, R. Kanetake\",\"doi\":\"10.1063/1.45938\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The vertical oscillation of an accretion disk surrounding a neutron star is studied by using the OPAL opacities. We have found that the vertical structure of the model disk is vibrationally unstable when we use new opacities instead of the Los Alamos opacities.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"118 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The evolution of X‐ray binaries\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.45938\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The evolution of X‐ray binaries","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1063/1.45938","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The vertical oscillation of an accretion disk surrounding a neutron star is studied by using the OPAL opacities. We have found that the vertical structure of the model disk is vibrationally unstable when we use new opacities instead of the Los Alamos opacities.
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