A radio-detected type Ia supernova with helium-rich circumstellar material

Type Ia supernovae (SNe Ia) are thermonuclear explosions of degenerate white dwarf stars destabilized by mass accretion from a companion star(1), but the nature of their progenitors remains poorly understood. A way to discriminate between progenitor systems is through radio observations; a non-degen...

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Detalles Bibliográficos
Autores principales: Kool, Erik C., Johansson, Joel, Sollerman, Jesper, Moldón, Javier, Moriya, Takashi J., Mattila, Seppo, Schulze, Steve, Chomiuk, Laura, Pérez-Torres, Miguel, Harris, Chelsea, Lundqvist, Peter, Graham, Matthew, Yang, Sheng, Perley, Daniel A., Strotjohann, Nora Linn, Fremling, Christoffer, Gal-Yam, Avishay, Lezmy, Jeremy, Maguire, Kate, Omand, Conor, Smith, Mathew, Andreoni, Igor, Bellm, Eric C., Bloom, Joshua S., De, Kishalay, Groom, Steven L., Kasliwal, Mansi M., Masci, Frank J., Medford, Michael S., Park, Sungmin, Purdum, Josiah, Reynolds, Thomas M., Riddle, Reed, Robert, Estelle, Ryder, Stuart D., Sharma, Yashvi, Stern, Daniel
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10191849/
https://www.ncbi.nlm.nih.gov/pubmed/37198310
http://dx.doi.org/10.1038/s41586-023-05916-w

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10191849/
https://www.ncbi.nlm.nih.gov/pubmed/37198310
http://dx.doi.org/10.1038/s41586-023-05916-w

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