{"title":"星际介质中远红外精细结构线的观测","authors":"D. Watson, J. Storey, C. Townes","doi":"10.1109/ICSWA.1979.9335408","DOIUrl":null,"url":null,"abstract":"Fine structure lines in the far-infrared have many simple properties that make them useful tools for diagnosing astrophysical plasmas. The line ratios are sensitive and accurate probes of density, elemental abundances, and ionization structure; also, line shapes and Doppler shifts have proven handy in studies of gross dynamics of H II regions and galaxies. These lines have several analytical and practical advantages over spectral features in the optical and radio regions for measuring certain parameters of ionized regions.","PeriodicalId":216123,"journal":{"name":"1979 International Conference on Submillimeter Waves and Their Applications","volume":"16 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1979-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Observations of Far-Infrared Fine Structure Lines in the Interstellar Medium\",\"authors\":\"D. Watson, J. Storey, C. Townes\",\"doi\":\"10.1109/ICSWA.1979.9335408\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Fine structure lines in the far-infrared have many simple properties that make them useful tools for diagnosing astrophysical plasmas. The line ratios are sensitive and accurate probes of density, elemental abundances, and ionization structure; also, line shapes and Doppler shifts have proven handy in studies of gross dynamics of H II regions and galaxies. These lines have several analytical and practical advantages over spectral features in the optical and radio regions for measuring certain parameters of ionized regions.\",\"PeriodicalId\":216123,\"journal\":{\"name\":\"1979 International Conference on Submillimeter Waves and Their Applications\",\"volume\":\"16 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1979-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"1979 International Conference on Submillimeter Waves and Their Applications\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/ICSWA.1979.9335408\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"1979 International Conference on Submillimeter Waves and Their Applications","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ICSWA.1979.9335408","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Observations of Far-Infrared Fine Structure Lines in the Interstellar Medium
Fine structure lines in the far-infrared have many simple properties that make them useful tools for diagnosing astrophysical plasmas. The line ratios are sensitive and accurate probes of density, elemental abundances, and ionization structure; also, line shapes and Doppler shifts have proven handy in studies of gross dynamics of H II regions and galaxies. These lines have several analytical and practical advantages over spectral features in the optical and radio regions for measuring certain parameters of ionized regions.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
