{"title":"对空间飞行器在Be恒星中可观测到的[Fe II]、[Fe III]、[Ni II]和[Ni III]禁止条纹的考虑","authors":"J. Swings","doi":"10.3406/barb.1965.65161","DOIUrl":null,"url":null,"abstract":"The strongest forbidden transitions of [Fe II], [Fe III], [Ni II] and [Ni III] have been computed as a preliminary step in the preparation of spectroscopic observations of bright line stars with space vehicles. Several predicted forbidden emissions play certainly an important role, especially in the infrared region.","PeriodicalId":296277,"journal":{"name":"Bulletin de la Classe des sciences","volume":"20 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Considérations sur les raies interdites de [Fe II], [Fe III], [Ni II] et [Ni III] observables dans les étoiles Be, par véhicules spatiaux\",\"authors\":\"J. Swings\",\"doi\":\"10.3406/barb.1965.65161\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The strongest forbidden transitions of [Fe II], [Fe III], [Ni II] and [Ni III] have been computed as a preliminary step in the preparation of spectroscopic observations of bright line stars with space vehicles. Several predicted forbidden emissions play certainly an important role, especially in the infrared region.\",\"PeriodicalId\":296277,\"journal\":{\"name\":\"Bulletin de la Classe des sciences\",\"volume\":\"20 1\",\"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\":\"Bulletin de la Classe des sciences\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.3406/barb.1965.65161\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin de la Classe des sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3406/barb.1965.65161","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Considérations sur les raies interdites de [Fe II], [Fe III], [Ni II] et [Ni III] observables dans les étoiles Be, par véhicules spatiaux
The strongest forbidden transitions of [Fe II], [Fe III], [Ni II] and [Ni III] have been computed as a preliminary step in the preparation of spectroscopic observations of bright line stars with space vehicles. Several predicted forbidden emissions play certainly an important role, especially in the infrared region.