{"title":"银河系中心的恒星群","authors":"M. Rieke","doi":"10.1063/1.43954","DOIUrl":null,"url":null,"abstract":"Near‐infrared imaging and spectroscopy have revealed a rich collection of stars whose character are now being understood as the result of several epochs of star formation. The collection of objects known as IRS16 may be intermediate temperature supergiants which need not contribute significantly to the ionizing radiation present in the central few parsecs.","PeriodicalId":310353,"journal":{"name":"Back to the Galaxy","volume":"10 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2008-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Stellar populations at the galactic center\",\"authors\":\"M. Rieke\",\"doi\":\"10.1063/1.43954\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Near‐infrared imaging and spectroscopy have revealed a rich collection of stars whose character are now being understood as the result of several epochs of star formation. The collection of objects known as IRS16 may be intermediate temperature supergiants which need not contribute significantly to the ionizing radiation present in the central few parsecs.\",\"PeriodicalId\":310353,\"journal\":{\"name\":\"Back to the Galaxy\",\"volume\":\"10 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2008-05-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Back to the Galaxy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1063/1.43954\",\"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/10.1063/1.43954","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Near‐infrared imaging and spectroscopy have revealed a rich collection of stars whose character are now being understood as the result of several epochs of star formation. The collection of objects known as IRS16 may be intermediate temperature supergiants which need not contribute significantly to the ionizing radiation present in the central few parsecs.
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