20 citations · 20 across the 1 of their papers we have counts for
10 papers
The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy
Luqian Wang, Douglas R. Gies, Geraldine J. Peters +4
The B-emission line stars are rapid rotators that were probably spun up by mass and angular momentum accretion through mass transfer in an interacting binary. Mass transfer will st…
Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
Elizabeth Berzin, Amy Secunda, Renyue Cen +2
While most simulations of the epoch of reionization have focused on single-stellar populations in star-forming dwarf galaxies, products of binary evolution are expected to signific…
Delayed Photons from Binary Evolution Help Reionize the Universe
Amy Secunda, Renyue Cen, Taysun Kimm +2
High-resolution numerical simulations including feedback and aimed at calculating the escape fraction (fesc) of hydrogen-ionizing photons often assume stellar radiation based on si…
The expansion of stripped-envelope stars: consequences for supernovae and gravitational-wave progenitors
E. Laplace, Y. Götberg, S. E. de Mink +2
Massive binaries that merge as compact objects are the progenitors of gravitational-wave sources. Most of these binaries experience one or more phases of mass transfer, during whic…
Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection
M. Renzo, R. J. Farmer, S. Justham +3
Gravitational-wave detections are now probing the black hole (BH) mass distribution, including the predicted pair-instability mass gap. These data require robust quantitative predi…
Predictions for the hydrogen-free ejecta of pulsational pair-instability supernovae
M. Renzo, R. Farmer, S. Justham +5
Present time-domain astronomy efforts will unveil a variety of rare transients. We focus here on pulsational pair-instability evolution, which can result in signatures observable w…