{"title":"吸积x射线脉冲星的性质","authors":"A. Parmar","doi":"10.1063/1.45982","DOIUrl":null,"url":null,"abstract":"The properties of accreting x‐ray pulsars are reviewed paying particular attention to their pulse and orbital periods and high‐energy x‐ray spectra. The importance of making broad‐band x‐ray measurements of these systems is demonstrated.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"5 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"The properties of accreting x‐ray pulsars\",\"authors\":\"A. Parmar\",\"doi\":\"10.1063/1.45982\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The properties of accreting x‐ray pulsars are reviewed paying particular attention to their pulse and orbital periods and high‐energy x‐ray spectra. The importance of making broad‐band x‐ray measurements of these systems is demonstrated.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"5 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The evolution of X‐ray binaries\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.45982\",\"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/10.1063/1.45982","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The properties of accreting x‐ray pulsars are reviewed paying particular attention to their pulse and orbital periods and high‐energy x‐ray spectra. The importance of making broad‐band x‐ray measurements of these systems is demonstrated.
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