123 citations · 723 across the 25 of their papers we have counts for
6 papers · 1 filter
Stellar Wind Yields of Very Massive Stars
Erin R. Higgins, Jorick S. Vink, Raphael Hirschi +2
The most massive stars provide an essential source of recycled material for young clusters and galaxies. While very massive stars (VMS, M>100M) are relatively rare compared to O st…
Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
James D. Keegans, Chris L. Fryer, Samuel W. Jones +6
Massive-star binaries can undergo a phase where one of the two stars expands during its advanced evolutionary stage as a giant and envelops its companion, ejecting the hydrogen env…
Non standard s-process in massive rotating stars. Yields of models at
Arthur Choplin, Raphael Hirschi, Georges Meynet +3
Recent studies show that rotation significantly affects the s-process in massive stars. We provide tables of yields for non-rotating and rotating massive stars between 10 and 150 $…
Spectroscopy of Ne for the thermonuclear O()Ne and F()O reaction rates
A. Parikh, A. M. Laird, N. de Séréville +10
Uncertainties in the thermonuclear rates of the O()Ne and F()O reactions affect model predictions of light curves from type I X-ray bursts and…
Constraining nova observables: direct measurements of resonance strengths in 33S(p,γ)34Cl
J. Fallis, A. Parikh, P. F. Bertone +32
The 33S(p,γ)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abu…
Is γ-ray emission from novae affected by interference effects in the 18F(p,α)15O reaction?
A. M. Laird, A. Parikh, A. St. J. Murphy +14
The 18F(p,α)15O reaction rate is crucial for constraining model predictions of the γ-ray observable radioisotope 18F produced in novae. The determination of this rate is challengin…