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- W1656971147 abstract "We have written a 3D radiative transfer code that computes emerging spectra and intensity maps. We derive from radiative hydrodynamic (RHD) simulations of RSG stars carried out with CO 5 BOLD (Freytag et al. 2002) observables expected for red supergiant stars (RSG) especially for interferometric observations, with emphasis on small scale structures. We show that the convection-related surface structures are detectable in the H band with today’s interferometers and that the diameter measurement should not be too dependent on the adopted model. The simulations are a great improvement over parametric models for the interpretation of interferometric observations." @default.
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- W1656971147 date "2007-07-01" @default.
- W1656971147 modified "2023-09-27" @default.
- W1656971147 title "Atmospheric dynamics of red supergiant stars and applications to Interferometry" @default.
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- W1656971147 hasPublicationYear "2007" @default.
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