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210 papers
OGLE-BLAP-009 -- A Case Study for the Properties and Evolution of Blue Large-Amplitude Pulsators
Corey W. Bradshaw, Matti Dorsch, Thomas Kupfer +5
Blue large-amplitude pulsators (BLAPs) make up a rare class of hot pulsating stars with effective temperatures of 30,000 K and surface gravities of 4.0 - 5.0 dex (cgs). Th…
The Asteroseismological Richness of RCB and dLHdC Stars
Tin Long Sunny Wong, Lars Bildsten
RCB stars are solar-mass objects that can exhibit large periods of extinction from dust ejection episodes. Many exhibit semiregular pulsations in the rang…
The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
Joel C. Zinn, Marc H. Pinsonneault, Lars Bildsten +1
Although stellar radii from asteroseismic scaling relations agree at the percent level with independent estimates for main sequence and most first-ascent red giant branch stars, th…
Turbulence Supported Massive Star Envelopes
William Schultz, Lars Bildsten, Yan-Fei Jiang
The outer envelopes of massive () stars exhibit large increases in opacities from forests of lines and ionization transitions (particularly from iron and hel…
Dynamical He Flashes in Double White Dwarf Binaries
Tin Long Sunny Wong, Lars Bildsten
The detonation of an overlying helium layer on a carbon-oxygen (CO) white dwarf (WD) can detonate the CO WD and create a thermonuclear supernova (SN).…
Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
Christopher E. O'Connor, Lars Bildsten, Matteo Cantiello +1
About ten percent of Sun-like (-) stars will engulf a - planet as they expand during the red giant branch (RGB) or asymptotic giant branch (AGB) phas…