no code implementations • 11 Mar 2021 • Shing-Chi Leung, Jim Fuller, Ken'ichi Nomoto
The fast rise in luminosity of this SN (spectroscopically classified as a broad-lined Type Ic SN), indicates that the ejecta interacts with a dense circumstellar medium (CSM), while an additional energy source such as $^{56}$Ni-decay is required to explain the late-time light curve.
High Energy Astrophysical Phenomena
no code implementations • 3 Sep 2020 • Shelley J. Cheng, Jim Fuller, Zhao Guo, Holger Lehman, Kelly Hambleton
Finally, we apply tidal theories to stellar structure models of each system to determine whether chance resonances can be responsible for the observed tidally excited oscillations, or whether a resonance locking process is at work.
Solar and Stellar Astrophysics
