{"title":"探测环面几何的一种方法","authors":"Chris Simpson","doi":"10.1016/0083-6656(95)00101-8","DOIUrl":null,"url":null,"abstract":"<div><p>I propose a method of inferring the geometry of the obscuring material in radio-loud active galaxies by examining the relationship between the inferred nuclear extinction and the core-to-lobe radio flux ratio. I use Monte Carlo simulations to estimate the quality of data expected from such a project and examine its usefulness in discriminating between alternative structures.</p></div>","PeriodicalId":101275,"journal":{"name":"Vistas in Astronomy","volume":"40 1","pages":"Pages 57-61"},"PeriodicalIF":0.0000,"publicationDate":"1996-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0083-6656(95)00101-8","citationCount":"4","resultStr":"{\"title\":\"A method of probing the torus geometry?\",\"authors\":\"Chris Simpson\",\"doi\":\"10.1016/0083-6656(95)00101-8\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>I propose a method of inferring the geometry of the obscuring material in radio-loud active galaxies by examining the relationship between the inferred nuclear extinction and the core-to-lobe radio flux ratio. I use Monte Carlo simulations to estimate the quality of data expected from such a project and examine its usefulness in discriminating between alternative structures.</p></div>\",\"PeriodicalId\":101275,\"journal\":{\"name\":\"Vistas in Astronomy\",\"volume\":\"40 1\",\"pages\":\"Pages 57-61\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1996-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/0083-6656(95)00101-8\",\"citationCount\":\"4\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Vistas in Astronomy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/0083665695001018\",\"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/0083665695001018","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
I propose a method of inferring the geometry of the obscuring material in radio-loud active galaxies by examining the relationship between the inferred nuclear extinction and the core-to-lobe radio flux ratio. I use Monte Carlo simulations to estimate the quality of data expected from such a project and examine its usefulness in discriminating between alternative structures.
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