no code implementations • 16 Feb 2021 • Ken J. Shen, Stéphane Blondin, Daniel Kasen, Luc Dessart, Dean M. Townsley, Samuel Boos, D. John Hillier
Type Ia supernovae (SNe Ia) span a range of luminosities and timescales, from rapidly evolving subluminous to slowly evolving overluminous subtypes.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
no code implementations • 29 Jan 2021 • Samuel J. Boos, Dean M. Townsley, Ken J. Shen, Spencer Caldwell, Broxton J. Miles
Despite the importance of Type Ia supernovae (SNe Ia) throughout astronomy, the precise progenitor systems and explosion mechanisms that drive SNe Ia are still unknown.
High Energy Astrophysical Phenomena
1 code implementation • 12 Oct 2020 • Keto D. Zhang, WeiKang Zheng, Thomas de Jaeger, Benjamin E. Stahl, Thomas G. Brink, Xuhui Han, Daniel Kasen, Ken J. Shen, Kevin Tang, Alexei V. Filippenko
In the two cases we consider, 35\% of SNe Ia are considered to be asymmetric in Case 1, and all SNe Ia are asymmetric in Case 2.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics
