{"title":"南半球几个HII区域的锯齿型激波锋","authors":"A. Gyulbudaghian","doi":"10.52526/25792776-2019.66.1-20","DOIUrl":null,"url":null,"abstract":"Radiation shock fronts at the heads of non adiabatic cooling jets are considered. Decay of these shock fronts leads to the origin of groups of HH objects, and of groups of bright condensations in the jets expelled from the nuclei of galaxies, e.g. from the nucleus of NGC5128. Several examples of saw-type radiation shock fronts, found in the Southern Hemisphere, are presented.","PeriodicalId":412578,"journal":{"name":"Communications of the Byurakan Astrophysical Observatory","volume":"130 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Saw-type shock fronts in several HII regions of southern hemisphere\",\"authors\":\"A. Gyulbudaghian\",\"doi\":\"10.52526/25792776-2019.66.1-20\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Radiation shock fronts at the heads of non adiabatic cooling jets are considered. Decay of these shock fronts leads to the origin of groups of HH objects, and of groups of bright condensations in the jets expelled from the nuclei of galaxies, e.g. from the nucleus of NGC5128. Several examples of saw-type radiation shock fronts, found in the Southern Hemisphere, are presented.\",\"PeriodicalId\":412578,\"journal\":{\"name\":\"Communications of the Byurakan Astrophysical Observatory\",\"volume\":\"130 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Communications of the Byurakan Astrophysical Observatory\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.52526/25792776-2019.66.1-20\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Communications of the Byurakan Astrophysical Observatory","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.52526/25792776-2019.66.1-20","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Saw-type shock fronts in several HII regions of southern hemisphere
Radiation shock fronts at the heads of non adiabatic cooling jets are considered. Decay of these shock fronts leads to the origin of groups of HH objects, and of groups of bright condensations in the jets expelled from the nuclei of galaxies, e.g. from the nucleus of NGC5128. Several examples of saw-type radiation shock fronts, found in the Southern Hemisphere, are presented.
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