J. Weiland, M. Hauser, T. Kelsall, E. Dwek, S. Moseley, R. Silverberg, M. Mitra, N. Odegard, W. Spiesman, T. J. Sodroski, S. W. Stemwedel, H. Freudenreich, C. Lisse
{"title":"银河凸出的远距离观测","authors":"J. Weiland, M. Hauser, T. Kelsall, E. Dwek, S. Moseley, R. Silverberg, M. Mitra, N. Odegard, W. Spiesman, T. J. Sodroski, S. W. Stemwedel, H. Freudenreich, C. Lisse","doi":"10.1063/1.44023","DOIUrl":null,"url":null,"abstract":"Near‐infrared observations of the Galactic bulge from the Diffuse Infrared Background Experiment (DIRBE) on‐board NASA’s Cosmic Background Explorer (COBE) satellite are discussed. Emphasis is placed on preliminary analysis of asymmetries in the brightness distribution of the bulge, and the implications for the presence of a stellar bar in the bulge region.","PeriodicalId":310353,"journal":{"name":"Back to the Galaxy","volume":"79 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Dirbe observations of the Galactic bulge\",\"authors\":\"J. Weiland, M. Hauser, T. Kelsall, E. Dwek, S. Moseley, R. Silverberg, M. Mitra, N. Odegard, W. Spiesman, T. J. Sodroski, S. W. Stemwedel, H. Freudenreich, C. Lisse\",\"doi\":\"10.1063/1.44023\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Near‐infrared observations of the Galactic bulge from the Diffuse Infrared Background Experiment (DIRBE) on‐board NASA’s Cosmic Background Explorer (COBE) satellite are discussed. Emphasis is placed on preliminary analysis of asymmetries in the brightness distribution of the bulge, and the implications for the presence of a stellar bar in the bulge region.\",\"PeriodicalId\":310353,\"journal\":{\"name\":\"Back to the Galaxy\",\"volume\":\"79 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Back to the Galaxy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.44023\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Back to the Galaxy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1063/1.44023","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Near‐infrared observations of the Galactic bulge from the Diffuse Infrared Background Experiment (DIRBE) on‐board NASA’s Cosmic Background Explorer (COBE) satellite are discussed. Emphasis is placed on preliminary analysis of asymmetries in the brightness distribution of the bulge, and the implications for the presence of a stellar bar in the bulge region.