Gaia17biu/SN 2017egm in NGC 3191:The Closest Hydrogen-poor Superluminous Supernova to Date Is in a 'Normal,' Massive, Metal-rich Spiral Galaxy

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OAIster

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Bose , S , Dong , S , Pastorello , A , Filippenko , A V , Kochanek , C S , Mauerhan , J , Romero-Canizales , C , Brink , T G , Chen , P , Prieto , J L , Post , R , Ashall , C , Grupe , D , Tomasella , L , Benetti , S , Shappee , B J , Stanek , K Z , Cai , Z , Falco , E , Lundqvist , P , Mattila , S , Mutel , R , Ochner , P , Pooley , D , Stritzinger , M D , Villanueva , S J , Zheng , W , Beswick , R J , Brown , P J , Cappellaro , E , Davis , S , Fraser , M , de Jaeger , T , Elias-Rosa , N , Gall , C , Gaudi , B S , Herczeg , G J , Hestenes , J , Holoien , T W -S , Hosseinzadeh , G , Hsiao , E Y , Hu , S , Jaejin , S , Jeffers , B , Koff , R A , Kumar , S , Kurtenkov , A , Lau , M W , Prentice , S , Reynolds , T , Rudy , R J , Shahbandeh , M , Somero , A , Stassun , K G , Thompson , T A , Valenti , S , Woo , J-H & Yunus , S 2018 , ' Gaia17biu/SN 2017egm in NGC 3191 : The Closest Hydrogen-poor Superluminous Supernova to Date Is in a "Normal," Massive, Metal-rich Spiral Galaxy ' , Astrophysical Journal , vol. 853 , no. 1 , 57 .

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English

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Electronic Resource

Accession number :

edsoai.on1322714148

Document Type :

Electronic Resource