13 research outputs found
Hydrodynamical model atmospheres and 3D spectral synthesis
Full text linkWe discuss three issues in the context of three-dimensional (3D)
hydrodynamical model atmospheres for late-type stars, related to spectral line
shifts, radiative transfer in metal-poor 3D models, and the solar oxygen
abundance. We include a brief overview about the model construction, taking the
radiation-hydrodynamics code CO5BOLD (COnservative COde for the COmputation of
COmpressible COnvection in a BOx of L Dimensions with L=2,3) and the related
spectral synthesis package Linfor3D as examples.Comment: 6 pages, 2 figures, to appear in the Proceedings of the
ESO/Lisbon/Aveiro Workshop "Precision Spectroscopy in Astrophysics", eds. L.
Pasquini, M. Romaniello, N.C. Santos, and A. Correi
The formation of hot subdwarf stars and its implications for the UV-upturn phenomenon of elliptical galaxies
No full textComparative effects of water immersion pretreatment on three different acute pancreatitis models in rats
No full textCoupling and control in coherently driven and asymmetrically synchronized hybrid electron-nuclear spin system
No full text
