{"title":"BQ cameloparadalis的六年光度测定- V0332+53的光学对应物","authors":"T. Mazeh, H. Mendelson","doi":"10.1063/1.46024","DOIUrl":null,"url":null,"abstract":"We report on the results of V, R, I photometry of BQ Cam—the optical counterpart of the transient x‐ray pulsar V0332+53, during the years 1985–91. Throughout this period we have detected a long‐term modulation correlated with the last observed x‐ray eruption. Similar long‐term modulation and correlation were observed in 4U0115+63—another Be‐star x‐ray source. We discussed briefly two scenarios for the optical modulation, with and without a possible large mediatory disc around the neutron star.","PeriodicalId":101857,"journal":{"name":"The evolution of X‐ray binaries","volume":"81 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Six‐year photometry of BQ Cameloparadalis—The optical counterpart of V0332+53\",\"authors\":\"T. Mazeh, H. Mendelson\",\"doi\":\"10.1063/1.46024\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We report on the results of V, R, I photometry of BQ Cam—the optical counterpart of the transient x‐ray pulsar V0332+53, during the years 1985–91. Throughout this period we have detected a long‐term modulation correlated with the last observed x‐ray eruption. Similar long‐term modulation and correlation were observed in 4U0115+63—another Be‐star x‐ray source. We discussed briefly two scenarios for the optical modulation, with and without a possible large mediatory disc around the neutron star.\",\"PeriodicalId\":101857,\"journal\":{\"name\":\"The evolution of X‐ray binaries\",\"volume\":\"81 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/10.1063/1.46024\",\"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/10.1063/1.46024","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Six‐year photometry of BQ Cameloparadalis—The optical counterpart of V0332+53
We report on the results of V, R, I photometry of BQ Cam—the optical counterpart of the transient x‐ray pulsar V0332+53, during the years 1985–91. Throughout this period we have detected a long‐term modulation correlated with the last observed x‐ray eruption. Similar long‐term modulation and correlation were observed in 4U0115+63—another Be‐star x‐ray source. We discussed briefly two scenarios for the optical modulation, with and without a possible large mediatory disc around the neutron star.
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
