{"title":"x射线双星的光谱诊断和吸积盘日冕再处理","authors":"T. Kallman","doi":"10.1063/1.46001","DOIUrl":null,"url":null,"abstract":"Emission lines are valuable probes of the conditions in the accretion flows associated with binary x‐ray sources. In this review I describe examples of emission lines in different spectral bands, review the observations, and discuss what they indicate about the conditions in binary x‐ray sources. These lines are interpreted using an x‐ray illuminated accretion disk model; the structure and dynamics of the heated disk, its spectral signatures, and the major unsolved theoretical issues surrounding them are discussed.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"30 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Spectral diagnostics and accretion disk corona reprocessing in x‐ray binaries\",\"authors\":\"T. Kallman\",\"doi\":\"10.1063/1.46001\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Emission lines are valuable probes of the conditions in the accretion flows associated with binary x‐ray sources. In this review I describe examples of emission lines in different spectral bands, review the observations, and discuss what they indicate about the conditions in binary x‐ray sources. These lines are interpreted using an x‐ray illuminated accretion disk model; the structure and dynamics of the heated disk, its spectral signatures, and the major unsolved theoretical issues surrounding them are discussed.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"30 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/10.1063/1.46001\",\"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/10.1063/1.46001","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Spectral diagnostics and accretion disk corona reprocessing in x‐ray binaries
Emission lines are valuable probes of the conditions in the accretion flows associated with binary x‐ray sources. In this review I describe examples of emission lines in different spectral bands, review the observations, and discuss what they indicate about the conditions in binary x‐ray sources. These lines are interpreted using an x‐ray illuminated accretion disk model; the structure and dynamics of the heated disk, its spectral signatures, and the major unsolved theoretical issues surrounding them are discussed.
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