{"title":"星周包络的傅里叶变换光谱学","authors":"J. J. Ready","doi":"10.1364/hrfts.1989.tua6","DOIUrl":null,"url":null,"abstract":"In the dusty circumstellar envelopes that sometimes occur around carbon-rich giant stars, acetylenic chemistry is very active (Cernicharo, et al. 1987). The circumstellar dust, some carbon compound thought to have condensed in or near the stellar photosphere (Ridgway and Ready, 1988), plays several roles.","PeriodicalId":159025,"journal":{"name":"High Resolution Fourier Transform Spectroscopy","volume":"58 5-6","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Fourier Transform Spectroscopy of Circumstellar Envelopes\",\"authors\":\"J. J. Ready\",\"doi\":\"10.1364/hrfts.1989.tua6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In the dusty circumstellar envelopes that sometimes occur around carbon-rich giant stars, acetylenic chemistry is very active (Cernicharo, et al. 1987). The circumstellar dust, some carbon compound thought to have condensed in or near the stellar photosphere (Ridgway and Ready, 1988), plays several roles.\",\"PeriodicalId\":159025,\"journal\":{\"name\":\"High Resolution Fourier Transform Spectroscopy\",\"volume\":\"58 5-6\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"High Resolution Fourier Transform Spectroscopy\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1364/hrfts.1989.tua6\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"High Resolution Fourier Transform Spectroscopy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/hrfts.1989.tua6","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
在富含碳的巨星周围的星周尘埃包层中，乙炔化学非常活跃(Cernicharo, et al. 1987)。星周尘埃，一些碳化合物被认为是在恒星光球圈内或附近凝结的(Ridgway和Ready, 1988)，扮演着几个角色。
Fourier Transform Spectroscopy of Circumstellar Envelopes
In the dusty circumstellar envelopes that sometimes occur around carbon-rich giant stars, acetylenic chemistry is very active (Cernicharo, et al. 1987). The circumstellar dust, some carbon compound thought to have condensed in or near the stellar photosphere (Ridgway and Ready, 1988), plays several roles.
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