Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a ‘normal’ massive, metal-rich spiral galaxy
| Title | Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a ‘normal’ massive, metal-rich spiral galaxy |
| Publication Type | Journal Article |
| Authors | Bose, S, Dong, S, Pastorello, A, Filippenko, AV, Kochanek, CS, Mauerhan, J, Romero-Cañizales, C, Brink, T, Chen, P, Prieto, JL, Post, R, Ashall, C, Grupe, D, Tomasella, L, Benetti, S, Shappee, BJ, Stanek, KZ, Cai, Z, Falco, E, Lundqvist, P, Mattila, S, Mutel, R, Ochner, P, Pooley, D, Stritzinger, MD, Villanueva, Jr., S, Zheng, W-K, Beswick, RJ, Brown, PJ, Cappellaro, E, Davis, S, Fraser, M, de Jaeger, T, Elias-Rosa, N, Gall, C, Gaudi, BS, Herczeg, GJ, Hestenes, J, Holoien, TW-S, Hosseinzadeh, G, Hsiao, EY, Hu, S-M, Jaejin, S, Jeffers, B, Koff, RA, Kumar, S, Kurtenkov, A, Lau, MW, Prentice, S, Reynolds, T, Rudy, RJ, Shahbandeh, M, Somero, A, Stassun, KG, Thompson, TA, Valenti, S, Woo, J-H, Yunus, S |
English