Round Table Summary: Problems in Modelling Stellar Atmospheres
Top Cited Papers
- 1 January 2003
- journal article
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 210, 47-48
- https://doi.org/10.1017/s0074180900133248
Abstract
The aim of the Round Table (RT) ”Problems in modelling stellar atmospheres“ was that of giving a panoramic view of the state of art on the atmospheric models used to predict observations of stars from T to A spectral type, the Sun included.Keywords
This publication has 29 references indexed in Scilit:
- Mass-loss rate determination for the massive binary V444 Cygni using 3-D Monte-Carlo simulations of line and polarization variabilityAstronomy & Astrophysics, 2002
- Short characteristic integration of radiative transfer problems: Formal solution in two-dimensional slabsJournal of Quantitative Spectroscopy and Radiative Transfer, 1988
- Two-dimensional radiative transfer. I - Planar geometryThe Astrophysical Journal, 1978
- The Formation of Resonance Lines in Multidimensional Media. III. Interpolation Functions, Accuracy, and StabilityThe Astrophysical Journal, 1973
- The Formation of Resonance Lines in Multidimensional Media. II. Radiation Operators and Their Numerical RepresentationThe Astrophysical Journal, 1973
- The stellar atmospheres problemJournal of Quantitative Spectroscopy and Radiative Transfer, 1971
- The Formation of Resonance Lines in Multidimensional Media. I. Scaling Properties in Two DimensionsThe Astrophysical Journal, 1971
- The Monte Carlo technique applied to radiative transferJournal of Quantitative Spectroscopy and Radiative Transfer, 1969
- A solar spicule model based upon calcium II K line radiative transfer studiesSolar Physics, 1969
- Radiative transport in finite homogenous cylinders by the Monte Carlo techniqueJournal of Quantitative Spectroscopy and Radiative Transfer, 1969