{"title":"脉冲星射电光度的统计分析","authors":"Wang Zhen-ru, Qu Qin-yue, Lu Tan, Luo Liao-fu","doi":"10.1016/0146-6364(80)90051-1","DOIUrl":null,"url":null,"abstract":"<div><p>The results of statistical analyses of the radio luminsotiy of 81 pulsars obtained in this paper appear to be in favour of the view that the radio emission originates in regions close to the light cylinder. The various statistical relations given in TABLES 1 and 2 may provide some clues on the radio emission.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 2","pages":"Pages 202-206"},"PeriodicalIF":0.0000,"publicationDate":"1980-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90051-1","citationCount":"4","resultStr":"{\"title\":\"Statistical analysis of the radio luminosity of pulsars\",\"authors\":\"Wang Zhen-ru, Qu Qin-yue, Lu Tan, Luo Liao-fu\",\"doi\":\"10.1016/0146-6364(80)90051-1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>The results of statistical analyses of the radio luminsotiy of 81 pulsars obtained in this paper appear to be in favour of the view that the radio emission originates in regions close to the light cylinder. The various statistical relations given in TABLES 1 and 2 may provide some clues on the radio emission.</p></div>\",\"PeriodicalId\":100241,\"journal\":{\"name\":\"Chinese Astronomy\",\"volume\":\"4 2\",\"pages\":\"Pages 202-206\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1980-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0146-6364(80)90051-1\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Chinese Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0146636480900511\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0146636480900511","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Statistical analysis of the radio luminosity of pulsars
The results of statistical analyses of the radio luminsotiy of 81 pulsars obtained in this paper appear to be in favour of the view that the radio emission originates in regions close to the light cylinder. The various statistical relations given in TABLES 1 and 2 may provide some clues on the radio emission.