{"title":"GRS 1915+105射电辐射的准周期变化","authors":"Guy Pooley","doi":"10.1016/S0083-6656(96)00056-6","DOIUrl":null,"url":null,"abstract":"<div><p>Observations of the radio emission at 15 GHz from GRS 1915+105 were made with the Ryle telescope intermittently during late 1995, early 1996, at a time when the source was active in the X-ray band. Wide variations in flux density were observed during the flaring activity. On several days when the flux was at an intermediate level there appeared to be a quasi-periodic component with a period close to 40 min. Later observations show that other periods are also present.</p></div>","PeriodicalId":101275,"journal":{"name":"Vistas in Astronomy","volume":"41 1","pages":"Pages 17-19"},"PeriodicalIF":0.0000,"publicationDate":"1997-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S0083-6656(96)00056-6","citationCount":"1","resultStr":"{\"title\":\"Quasi-periodic variations in the radio emission from GRS 1915+105\",\"authors\":\"Guy Pooley\",\"doi\":\"10.1016/S0083-6656(96)00056-6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Observations of the radio emission at 15 GHz from GRS 1915+105 were made with the Ryle telescope intermittently during late 1995, early 1996, at a time when the source was active in the X-ray band. Wide variations in flux density were observed during the flaring activity. On several days when the flux was at an intermediate level there appeared to be a quasi-periodic component with a period close to 40 min. Later observations show that other periods are also present.</p></div>\",\"PeriodicalId\":101275,\"journal\":{\"name\":\"Vistas in Astronomy\",\"volume\":\"41 1\",\"pages\":\"Pages 17-19\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1997-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/S0083-6656(96)00056-6\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Vistas in Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0083665696000566\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Vistas in Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0083665696000566","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Quasi-periodic variations in the radio emission from GRS 1915+105
Observations of the radio emission at 15 GHz from GRS 1915+105 were made with the Ryle telescope intermittently during late 1995, early 1996, at a time when the source was active in the X-ray band. Wide variations in flux density were observed during the flaring activity. On several days when the flux was at an intermediate level there appeared to be a quasi-periodic component with a period close to 40 min. Later observations show that other periods are also present.