116 citations · 842 across the 28 of their papers we have counts for
58 papers
The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge
Ori D. Fox, Schuyler D. Van Dyk, Benjamin F. Williams +17
This Letter presents the detection of a source at the position of the Type Ib/c supernova (SN) 2013ge more than four years after the radioactive component is expected to have faded…
Physical Properties of the Host Galaxies of Ca-rich Transients
Y. Dong, D. Milisavljevic, J. Leja +8
Calcium-rich (Ca-rich) transients are a new class of supernovae (SNe) that are known for their comparatively rapid evolution, modest peak luminosities, and strong nebular calcium e…
A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
Taylor Jacovich, Daniel Patnaude, Pat Slane +4
Massive stars can shed material via steady, line-driven winds, eruptive outflows, or mass-transfer onto a binary companion. In the case of single stars, the mass is deposited by th…
The dust mass in Cassiopeia A from infrared and optical line flux differences
Maria Niculescu-Duvaz, Michael J. Barlow, Antonia Bevan +2
The large quantities of dust that have been found in a number of high redshift galaxies have led to suggestions that core-collapse supernovae (CCSNe) are the main sources of their…
Far UV and Optical Emissions from Three Very Large Supernova Remnants Located at Unusually High Galactic Latitudes
Robert A. Fesen, Marcel Drechsler, Kathryn E. Weil +9
Galactic supernova remnants (SNRs) with angular dimensions greater than a few degrees are relatively rare, as are remnants located more than ten degrees off the Galactic plane. Her…
SN 2014C: VLBI image shows a shell structure and decelerated expansion
Michael F. Bietenholz, Norbert Bartel, Atish Kamble +3
We report on new Very Long Baseline Interferometry radio measurements of supernova 2014C in the spiral galaxy NGC 7331, made with the European VLBI Network ~5 yr after the explosio…