179 citations · 557 across the 18 of their papers we have counts for
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Early supernova emission -- logarithmic corrections to the planar phase
Tamar Faran, Re'em Sari
When the shock wave generated in a supernova explosion breaks out of the stellar envelope, the first photons, typically in the X-ray to UV range, escape to the observer. Following…
The aspherical explosion of the Type IIP SN 2017gmr
T. Nagao, A. Cikota, F. Patat +7
Type IIP supernovae (SNe IIP), which represent the most common class of core-collapse (CC) SNe, show a rapid increase in continuum polarization just after entering the tail phase.…
SN 2017gmr: An energetic Type II-P supernova with asymmetries
Jennifer E. Andrews, D. J. Sand, S. Valenti +77
We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…
Recombination Effects on Supernova Light Curves
Tamar Faran, Tomer Goldfriend, Ehud Nakar +1
The light curves of type-II supernovae (SNe) are believed to be highly affected by recombination of hydrogen that takes place in their envelopes. In this work, we analytically inve…