SN 2017dio: A Type-Ic Supernova Exploding in a Hydrogen-rich Circumstellar Medium

SN 2017dio shows both spectral characteristics of a type-Ic supernova (SN) and signs of a hydrogen-rich circumstellar medium (CSM). Prominent, narrow emission lines of H and He are superposed on the continuum. Subsequent evolution revealed that the SN ejecta are interacting with the CSM. The initial...

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Detalles Bibliográficos
Autores principales: Kuncarayakti, Hanindyo, Maeda, Keiichi, Ashall, Christopher J., Prentice, Simon J., Mattila, Seppo, Kankare, Erkki, Fransson, Claes, Lundqvist, Peter, Pastorello, Andrea, Leloudas, Giorgos, Anderson, Joseph P., Benetti, Stefano, Bersten, Melina Cecilia, Cappellaro, Enrico, Cartier, Régis, Denneau, Larry, Della Valle, Massimo, Elias Rosa, Nancy, Folatelli, Gastón, Fraser, Morgan, Galbany, Lluís, Gall, Christa, Gal-Yam, Avishay, Gutiérrez, Claudia P., Hamanowicz, Aleksandra, Heinze, Ari, Inserra, Cosimo, Kangas, Tuomas, Mazzali, Paolo, Melandri, Andrea, Pignata, Giuliano, Rest, Armin, Reynolds, Thomas, Roy, Rupak, Smartt, Stephen J., Smith, Ken W., Sollerman, Jesper, Somero, Auni, Stalder, Brian, Stritzinger, Maximilian, Taddia, Francesco, Tomasella, Lina, Tonry, John, Weiland, Henry, Young, David R.
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2018
Materias:
Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Supernovae: general
Supernovae: individual (SN 2017dio)
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93601
https://iopscience.iop.org/article/10.3847/2041-8213/aaaa1a
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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