{"title":"SS433的岁差相位相关的x射线发射","authors":"W. Yuan, N. Kawai, M. Matsuoka","doi":"10.1063/1.46037","DOIUrl":null,"url":null,"abstract":"The evolution of x‐ray emission of SS433 over its precessional period gave an evidence to the existence of an alternative harder x‐ray emission region apart from the jets. The spectral fits with a two continuum component model involving such a hard x‐ray component gave further support to this scenario.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"82 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The precessional phase dependent x‐ray emission of SS433\",\"authors\":\"W. Yuan, N. Kawai, M. Matsuoka\",\"doi\":\"10.1063/1.46037\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The evolution of x‐ray emission of SS433 over its precessional period gave an evidence to the existence of an alternative harder x‐ray emission region apart from the jets. The spectral fits with a two continuum component model involving such a hard x‐ray component gave further support to this scenario.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"82 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/10.1063/1.46037\",\"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/10.1063/1.46037","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The precessional phase dependent x‐ray emission of SS433
The evolution of x‐ray emission of SS433 over its precessional period gave an evidence to the existence of an alternative harder x‐ray emission region apart from the jets. The spectral fits with a two continuum component model involving such a hard x‐ray component gave further support to this scenario.
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