C. Wilson, B. A. Harmon, R. Wilson, G. Fishman, C. Meegan, D. Chakrabarty, J. Grunsfeld, T. Prince, M. Finger, W. Paciesas, G. Pendleton
{"title":"BATSE observations of GS 0834‐430","authors":"C. Wilson, B. A. Harmon, R. Wilson, G. Fishman, C. Meegan, D. Chakrabarty, J. Grunsfeld, T. Prince, M. Finger, W. Paciesas, G. Pendleton","doi":"10.1063/1.44303","DOIUrl":null,"url":null,"abstract":"GS 0834‐430 has been observed in seven outbursts with the Large Area Detectors (LAD’s) of the Burst and Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory. We have fit observed pulse frequencies and total flux with a model that assumes binary motion and a relationship between the total flux and accretion induced torque. In addition, we have fit the first five harmonics of 4–6 day summed pulse profiles with a template pulse profile for each channel to detect changes in pulse shape. We present the history of the total flux and the pulsed frequency, pulse profiles, and orbital parameters.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"38 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1993-07-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The evolution of X‐ray binaries","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1063/1.44303","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
Abstract
GS 0834‐430 has been observed in seven outbursts with the Large Area Detectors (LAD’s) of the Burst and Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory. We have fit observed pulse frequencies and total flux with a model that assumes binary motion and a relationship between the total flux and accretion induced torque. In addition, we have fit the first five harmonics of 4–6 day summed pulse profiles with a template pulse profile for each channel to detect changes in pulse shape. We present the history of the total flux and the pulsed frequency, pulse profiles, and orbital parameters.
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