papers
Publications (16)
astro-ph2006
The mass loss of C-rich giants
J. Bergeat, L. Chevallier
astro-ph2007
Fast 2D non-LTE radiative modelling of prominences I. Numerical methods and benchmark results
L. Leger, L. Chevallier, F. Paletou
astro-ph2006
Integral equations for the H- X- and Y-functions
B. Rutily, L. Chevallier, J. Bergeat
astro-ph2006
The accuracy of the ALI method for solving the radiative transfer equation in stellar atmospheres
L. Chevallier, F. Paletou, B. Rutily
astro-ph2006
Thermalisation of electrons in a stellar atmosphere
L. Chevallier
astro-ph.IM2009
Thermal instability in X-ray photoionized media in Active Galactic Nuclei: II. Role of the thermal conduction in warm absorber
B. Czerny, L. Chevallier, A. C. Goncalves +2
astro-ph2006
The puzzle of the soft X-ray excess in AGN: absorption or reflection?
L. Chevallier, S. Collin, A. -M. Dumont +4
astro-ph2007
Response of the warm absorber cloud to a variable nuclear flux in active galactic nuclei
L. Chevallier, B. Czerny, A. Rozanska +1
astro-ph2006
The finite Laplace transform for solving a weakly singular integral equation occurring in transfer theory
B. Rutily, L. Chevallier
astro-ph2006
Exact vs. Gauss-Seidel non-LTE radiation transfer solutions
C. Quang, F. Paletou, L. Chevallier
astro-ph2006
A new model for the Warm Absorber in NGC 3783: a single medium in total pressure equilibrium
A. C. Goncalves, S. Collin, A. -M. Dumont +4
astro-ph2006
Radiative transfer in plane-parallel media and Cauchy integral equations II. The H-function
B. Rutily, J. Bergeat, L. Chevallier
astro-ph2006
Thermal instability in X-ray photoionized media in Active Galactic Nuclei: Influence on the gas structure and spectral features
A. C. Goncalves, S. Collin, A. -M. Dumont +1
astro-ph2006
On the accuracy of the ALI method for solving the radiative transfer equation
L. Chevallier, F. Paletou, B. Rutily
astro-ph2006
Radiative transfer in plane-parallel media and Cauchy integral equations III. The finite case
B. Rutily, L. Chevallier, J. Bergeat
astro-ph2005
Exact solution of the standard transfer problem in a stellar atmosphere
L. Chevallier, B. Rutily