{"title":"空间实验室用于远红外天文的氦冷却迈克尔逊干涉仪","authors":"S. Drapatz, R. Hofmann, R. Katterloher","doi":"10.1109/IRMM.1983.9126510","DOIUrl":null,"url":null,"abstract":"Spectroscopy of astronomical objects in the mid- and far-infrared region will contribute substantially to our understanding of basic astrophysical processes (e.g. formation of stars and galaxies). Today, a number of intense lines have been detected in the brightest sources (mainly HII regions) using airborne and balloon-borne telescopes with equipments at ambient temperatures.","PeriodicalId":314918,"journal":{"name":"1983 Eighth International Conference on Infrared and Millimeter Waves","volume":"41 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1983-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A helium cooled michelson interferometer for far infrared astronomy on spacelab\",\"authors\":\"S. Drapatz, R. Hofmann, R. Katterloher\",\"doi\":\"10.1109/IRMM.1983.9126510\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Spectroscopy of astronomical objects in the mid- and far-infrared region will contribute substantially to our understanding of basic astrophysical processes (e.g. formation of stars and galaxies). Today, a number of intense lines have been detected in the brightest sources (mainly HII regions) using airborne and balloon-borne telescopes with equipments at ambient temperatures.\",\"PeriodicalId\":314918,\"journal\":{\"name\":\"1983 Eighth International Conference on Infrared and Millimeter Waves\",\"volume\":\"41 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1983-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"1983 Eighth International Conference on Infrared and Millimeter Waves\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/IRMM.1983.9126510\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"1983 Eighth International Conference on Infrared and Millimeter Waves","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/IRMM.1983.9126510","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A helium cooled michelson interferometer for far infrared astronomy on spacelab
Spectroscopy of astronomical objects in the mid- and far-infrared region will contribute substantially to our understanding of basic astrophysical processes (e.g. formation of stars and galaxies). Today, a number of intense lines have been detected in the brightest sources (mainly HII regions) using airborne and balloon-borne telescopes with equipments at ambient temperatures.
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