M. Finger, L. Cominsky, R. Wilson, B. A. Harmon, G. Fishman
{"title":"A 0535+262的硬x射线观测","authors":"M. Finger, L. Cominsky, R. Wilson, B. A. Harmon, G. Fishman","doi":"10.1063/1.46032","DOIUrl":null,"url":null,"abstract":"Three outbursts of the x‐ray binary system A 0535+262 have been detected in the 20–120 keV energy range by the BATSE instrument onboard the Compton Gamma Ray Observatory. The system orbital parameters have been determined by a pulse timing analysis during data from these outbursts.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"11 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":"{\"title\":\"Hard x‐ray observations of A 0535+262\",\"authors\":\"M. Finger, L. Cominsky, R. Wilson, B. A. Harmon, G. Fishman\",\"doi\":\"10.1063/1.46032\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Three outbursts of the x‐ray binary system A 0535+262 have been detected in the 20–120 keV energy range by the BATSE instrument onboard the Compton Gamma Ray Observatory. The system orbital parameters have been determined by a pulse timing analysis during data from these outbursts.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"11 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-12\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The evolution of X‐ray binaries\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.46032\",\"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/10.1063/1.46032","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Three outbursts of the x‐ray binary system A 0535+262 have been detected in the 20–120 keV energy range by the BATSE instrument onboard the Compton Gamma Ray Observatory. The system orbital parameters have been determined by a pulse timing analysis during data from these outbursts.
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