Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Max Plank Institute for Astrophysics
MPA
ANU
Nordita
MPA-Garching, Germany
MPA Garching
Uppsala
Uppsala Astronomical Observatory, Sweden
RSAA, Mt. Stromlo Observatory
Max Planck Institute for Astrophysics, Postfach 1317, 85741 Garching bei München, Germany
Max-Planck-Institut für Astrophysik, Germany
Max Planck Institute for Astrophysics, Germany
Planetary Science Institute, The Australian National University, Canberra ACT 0200, Australia; Research School of Astronomy and Astrophysics, ANU, Australia
Research School of Astronomy and Astrophysics, Australian National University, Mt. Stromlo Observatory, Cotter Rd., Weston, ACT 2611, Australia
NORDITA, Blegdamsvej 17, DK-2100 Copenhagen Ø, Denmark
Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, ACT 2611, Australia
Mount Stromlo Obs., Australia
Institute for Astronomy and Space Physics, Box 515, 751 20, Uppsala, Sweden
NORDITA, Blegdamsvej 17, 2100 Copenhagen Ø, Denmark; Astronomiska observatoiret, Box 515, 751 20 Uppsala, Sweden
Astronomiska Observatoiret, Box 515, S-751 20 Uppsala, Sweden
Research School of Astronomy & Astrophysics, Cotter Road, Weston Creek, 2611, Australia ; Max Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741, Garching, Germany
Mt. Stromlo Obs.
Astronomiska observatoiret, Box 515, S-751 20 Uppsala, Sweden
Australian National University, Weston, Australia
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany School of Astronomy and Astrophysics, Mt. Stromlo Observatory, Cotter Rd., Weston, ACT 2611, Australia
MPA, Germany
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild Str. 1, Garching, Germany
Max Planck Institute for Astrophysics, Postfach 1317, D-85741 Garching bei München, Germany
Uppsala Astronomical Observatory
Astronomiska Obs
(Erratum) Line-blanketed model atmospheres for R Coronae Borealis stars and hydrogen-deficient carbon stars.
18O and the Origins of HdC and R CrB Stars
3D hydrodynamical model atmospheres of metal-poor stars: Evidence for a low primordial Li abundance
3D hydrodynamical model atmospheres: a tool to correct radial velocities and parallaxes for Gaia
3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis
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