Dynamic model atmospheres of AGB stars - III. Effects of frequency-dependent radiative transfer

By S. Höfner, R. Gautschy-Loidl, B. Aringer, U. Jørgensen. 2003

134 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/b92e08f9a911447a9631f4166e0ccf2c75c79ada

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In Astronomy and Astrophysics

Citations in the corpus

Mass loss of stars on the asymptotic giant branch (2018, unknown): “Mattsson et al. (2010) and Eriksson et al. (2014) presented the to-date most substantial grid of such models for C-rich AGB stars (based on the DARWIN code; Höfner et al. 2003, 2016).”
A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties (2008, background): “…for cool giants have been developed by Wood (1979) and Bowen (1988), and these were improved with time-dependent dust formation by Fleischer et al. (1992) and Höfner & Dorfi (1997), and further developed to include frequency-dependent radiative transfer by Höfner (1999) and Höfner et al. (2003).”
Production of dust by massive stars at high redshift (2011, background): “Detailed time-dependent dynamical models featuring a frequency-dependent treatment of the radiative transfer have successfully explained the mass-loss mechanism for C-stars (e.g.,Höfner et al, 2003; Höfner, 2006; Winters et al, 2000).”
Dust formation in the oxygen-rich AGB star IK Tauri (2015, methodology): “Therefore, our model provides a simplified description compared to more sophisticated A6, page 4 of 15 hydrodynamic models of the inner wind, which take into account the dust radiative feedback on the gas (e.g., Winters et al. 2000; Höfner et al. 2003; Woitke 2006).”
EVOLUTION OF MASSIVE STARS WITH PULSATION-DRIVEN SUPERWINDS DURING THE RED SUPERGIANT PHASE (2010, background): “…RSGs are unstable to radial pulsations driven by partial ionization of hydrogen in the outermost layers of the envelope (e.g. Li & Gong 1994), and pulsation is one of the most commonly invoked mechanisms for driving winds from cool stars (cf. Bowen 1988; Höfner et al. 2003; Neilson & Lester 2008).”
Too little radiation pressure on dust in the winds of oxygen-rich AGB stars (2006, result): “Similar results have been obtained by Höfner et al. (2003) and Helling & Jørgensen (1998), using a sparse opacity sampling technique with about 100 sampling points.”