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

2.9k citations

Showing 2012 · astro-ph.SRShow all

32 papers · 2 filters

astro-ph.SR2012★ 130 cited

The 12C + 12C reaction and the impact on nucleosynthesis in massive stars

M. Pignatari, R. Hirschi, M. Wiescher +7

Despite much effort in the past decades, the C-burning reaction rate is uncertain by several orders of magnitude, and the relative strength between the different channels 12C(12C,a…

astro-ph.SR2012★ 80 cited

Period and period change measurements for 143 SuperWASP eclipsing binary candidates near the short-period limit and discovery of a doubly eclipsing quadruple system

M. E. Lohr, A. J. Norton, U. C. Kolb +3

Building on previous work, a new search of the SuperWASP archive was carried out to identify eclipsing binary systems near the short-period limit. 143 candidate objects were detect…

astro-ph.SR2012★ 16 cited

MOA-2010-BLG-523: "Failed Planet" = RS CVn Star

A. Gould, J. C. Yee, I. A. Bond +116

The Galactic bulge source MOA-2010-BLG-523S exhibited short-term deviations from a standard microlensing lightcurve near the peak of an Amax ~ 265 high-magnification microlensing e…

astro-ph.SR2012★ 104 cited

Accurate spectroscopic parameters of WASP planet host stars

Amanda P. Doyle, B. Smalley, P. F. L. Maxted +8

We have made a detailed spectral analysis of eleven Wide Angle Search for Planets (WASP) planet host stars using high signal-to-noise (S/N) HARPS spectra. Our line list was careful…

astro-ph.SR2012★ 1 cited

Very Massive Stars and the Eddington Limit

Paul A. Crowther, R. Hirschi, Nolan R. Walborn +1

We use contemporary evolutionary models for Very Massive Stars (VMS) to assess whether the Eddington limit constrains the upper stellar mass limit. We also consider the interplay b…

astro-ph.SR2012★ 26 cited

Mass-loss predictions for evolved very metal-poor massive stars

Lianne Muijres, Jorick S. Vink, A. de Koter +3

(shortened) The first couple of stellar generations may have been massive, of order 100 Msun, and to have played a dominant role in galaxy formation and the chemical enrichment of…