activity
19942025
most citedAstrophysical Reaction Rates From Statistical Model Calculations

927 citations · 7k across the 78 of their papers we have counts for

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astro-ph.GA2015★ 43 cited

Mn abundances in the stars of the Galactic disc with metallicities -1.0 < [Fe/H] < 0.3

T. Mishenina, T. Gorbaneva, M. Pignatari +2

In this work we present and discuss the observations of the Mn abundances for 247 FGK dwarfs, located in the Galactic disc with metallicity -1<Fe/H]<+0.3. The observed stars belong…

astro-ph.HE2015

A primordial r-process?

T. Rauscher, J. H. Applegate, J. J. Cowan +2

Baryon density inhomogeneities in the early universe can give rise to a floor of heavy elements (up to ) produced in a primordial r-process with fission cycling. A pa…

astro-ph.HE2015

Primordial heavy element production

T. Rauscher, F. -K. Thielemann

A number of possible mechanisms have been suggested to generate density inhomogeneities in the early Universe which could survive until the onset of primordial nucleosynthesis and…

astro-ph.HE2015★ 8 cited

The LOFT perspective on neutron star thermonuclear bursts

J. J. M. in 't Zand, D. Altamirano, D. R. Ballantyne +31

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT f…

astro-ph.GA2015★ 190 cited

Galactic evolution of rapid neutron capture process abundances: the inhomogeneous approach

B. Wehmeyer, M. Pignatari, F. -K. Thielemann

For the origin of heavy r-process elements, different sources have been proposed, e.g., core-collapse supernovae or neutron star mergers. Old metal-poor stars carry the signature o…

astro-ph.SR2015★ 114 cited

Pushing 1D CCSNe to explosions: model and SN 1987A

A. Perego, M. Hempel, C. Fröhlich +5

We report on a method, PUSH, for triggering core-collapse supernova explosions of massive stars in spherical symmetry. We explore basic explosion properties and calibrate PUSH such…