{"title":"蜕变","authors":"Andrea Bonime-Blanc","doi":"10.4324/9780429287787-7","DOIUrl":null,"url":null,"abstract":"The stellar explosions known as supernovae are not simply brilliant signposts marking the transition from one stage of the stellar life cycle to the next. They hold clues to the very nature of massive stars, trigger (or disrupt) nearby star formation, affect the interstellar media and chemical evolution of their host galaxies, and serve as standard candles that trace the expansion history of the universe. But understanding these crucial roles requires understanding the complex geometrical nature of supernovae and the stellar systems that give rise to them.","PeriodicalId":135160,"journal":{"name":"Gloom to Boom","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2019-10-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Metamorphosis\",\"authors\":\"Andrea Bonime-Blanc\",\"doi\":\"10.4324/9780429287787-7\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The stellar explosions known as supernovae are not simply brilliant signposts marking the transition from one stage of the stellar life cycle to the next. They hold clues to the very nature of massive stars, trigger (or disrupt) nearby star formation, affect the interstellar media and chemical evolution of their host galaxies, and serve as standard candles that trace the expansion history of the universe. But understanding these crucial roles requires understanding the complex geometrical nature of supernovae and the stellar systems that give rise to them.\",\"PeriodicalId\":135160,\"journal\":{\"name\":\"Gloom to Boom\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-10-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Gloom to Boom\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.4324/9780429287787-7\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Gloom to Boom","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.4324/9780429287787-7","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The stellar explosions known as supernovae are not simply brilliant signposts marking the transition from one stage of the stellar life cycle to the next. They hold clues to the very nature of massive stars, trigger (or disrupt) nearby star formation, affect the interstellar media and chemical evolution of their host galaxies, and serve as standard candles that trace the expansion history of the universe. But understanding these crucial roles requires understanding the complex geometrical nature of supernovae and the stellar systems that give rise to them.