output
19952026
most citedDigital Twin: Enabling Technologies, Challenges and Open Research

2.9k citations

Showing 2017 · astro-ph.SRShow all

42 papers · 2 filters

astro-ph.SR2017★ 1 cited

The First 3D Simulations of Carbon Burning in a Massive Star

Andrea Cristini, Casey Meakin, Raphael Hirschi +3

We present the first detailed three-dimensional hydrodynamic implicit large eddy simulations of turbulent convection for carbon burning. The simulations start with an initial radia…

astro-ph.SR2017★ 53 cited

Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations

N. Nishimura, T. Rauscher, R. Hirschi +3

Thermonuclear supernovae originating from the explosion of a white dwarf accreting mass from a companion star have been suggested as a site for the production of nuclides. Such…

astro-ph.SR2017★ 73 cited

The Gaia-ESO Survey: open clusters in Gaia-DR1 - a way forward to stellar age calibration

S. Randich, E. Tognelli, R. Jackson +42

We describe the methodologies that, taking advantage of Gaia-DR1 and the Gaia-ESO Survey data, enable the comparison of observed open star cluster sequences with stellar evolutiona…

astro-ph.SR2017★ 44 cited

An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-Redshift AGB Analogs

M. L. Boyer, K. B. W. McQuinn, M. A. T. Groenewegen +13

The survey for DUST in Nearby Galaxies with Spitzer (DUSTiNGS) identified several candidate Asymptotic Giant Branch (AGB) stars in nearby dwarf galaxies and showed that dust can fo…

astro-ph.SR2017★ 10 cited

Evolutionary Constraints on the Long-period Subdwarf B Binary PG 1018-047

J. Deca, J. Vos, P. Németh +4

We have revisited the sdB+K-star long-period binary PG 1018-047 based on 20 new high-resolution VLT/UVES spectra that provided regular coverage over a period of more than 26 months…

astro-ph.SR2017★ 56 cited

Are some CEMP-s stars the daughters of spinstars?

Arthur Choplin, Raphael Hirschi, Georges Meynet +1

CEMP-s stars are long-lived low-mass stars with a very low iron content as well as overabundances of carbon and s-elements. Their peculiar chemical pattern is often explained by po…