activity
19972023
most citedHow Massive Single Stars End their Life

2.2k citations · 21.5k across the 170 of their papers we have counts for

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36 papers · 1 filter

astro-ph2008★ 45 cited

The Impact of Neutrino Magnetic Moments on the Evolution of Massive Stars

Alexander Heger, Alexander Friedland, Maurizio Giannotti +1

We explore the sensitivity of massive stars to neutrino magnetic moments. We find that the additional cooling due to the neutrino magnetic moments bring about qualitative changes t…

astro-ph2008★ 64 cited

Dependence of S-Process Nucleosynthesis in Massive Stars on Triple-Alpha and 12C(a,g)16O Reaction Rate Uncertainties

Clarisse Tur, Alexander Heger, Sam M. Austin

We have studied the sensitivity of s-process nucleosynthesis in massive stars to +/- 2 sigma variations in the rates of the triple alpha and 12C(a,g)16O reactions. We simulated the…

astro-ph2008★ 83 cited

Multiple ring nebulae around blue supergiants

S. M. Chita, N. Langer, A. J. van Marle +2

In the course of the life of a massive star, wind-wind interaction can give rise to the formation of circumstellar nebulae which are both predicted and observed in the nature. We p…

astro-ph2008★ 42 cited

The Molecular Hydrogen Deficit in Gamma-Ray Burst Afterglows

Daniel Whalen, Jason X. Prochaska, Alexander Heger +1

Recent analysis of five gamma-ray burst (GRB) afterglow spectra reveal the absence of molecular hydrogen absorption lines, a surprising result in light of their large neutral hydro…

astro-ph2007★ 116 cited

Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning

Alexander Heger, Andrew Cumming, Duncan K. Galloway +1

The X-ray burster GS 1826-24 shows extremely regular Type I X-ray bursts whose energetics and recurrence times agree well with thermonuclear ignition models. We present calculation…

astro-ph2007★ 1 cited

The Metallicity Dependence of Wolf-Rayet Mass Loss

A. J. Onifer, A. Heger, J. Abdallah

We produce models of early WN, WC, and WO stars as a function of metallicity Z using an analytic CAK-type approach. At log(Z / Z_sun) >= -2 both WN and WC stars have the approximat…