M. Stollberg, W. Paciesas, M. Finger, G. Fishman, R. Wilson, B. A. Harmon, C. Wilson
{"title":"用BATSE对EXO 2030+375的最新观测","authors":"M. Stollberg, W. Paciesas, M. Finger, G. Fishman, R. Wilson, B. A. Harmon, C. Wilson","doi":"10.1063/1.46018","DOIUrl":null,"url":null,"abstract":"The transient x‐ray pulsar EXO 2030+375 has been detected in the Large Area Detectors (LADs) of BATSE during twelve outbursts from February 1992 to July 1993. These data have been fit to a model of the pulsar’s rotational phase which assumes an independent torque for each outburst. An intensity history, a pulse period history, a pulsed fraction, and the latest orbit parameters resulting from this fit are presented.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"52 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Recent observations of EXO 2030+375 with BATSE\",\"authors\":\"M. Stollberg, W. Paciesas, M. Finger, G. Fishman, R. Wilson, B. A. Harmon, C. Wilson\",\"doi\":\"10.1063/1.46018\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The transient x‐ray pulsar EXO 2030+375 has been detected in the Large Area Detectors (LADs) of BATSE during twelve outbursts from February 1992 to July 1993. These data have been fit to a model of the pulsar’s rotational phase which assumes an independent torque for each outburst. An intensity history, a pulse period history, a pulsed fraction, and the latest orbit parameters resulting from this fit are presented.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"52 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/10.1063/1.46018\",\"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/10.1063/1.46018","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The transient x‐ray pulsar EXO 2030+375 has been detected in the Large Area Detectors (LADs) of BATSE during twelve outbursts from February 1992 to July 1993. These data have been fit to a model of the pulsar’s rotational phase which assumes an independent torque for each outburst. An intensity history, a pulse period history, a pulsed fraction, and the latest orbit parameters resulting from this fit are presented.
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