Applications of

Radiative Transfer

to stellar and planetary atmospheres
Tenerife, Spain - 13-17 Nov. 2017

Lecturers & Topics


Fundamental physical aspects of radiative transfer

Artemio Herrero (Email)
Instituto de Astrofísica de Canarias & Dpto. de Astrofísica , Univ. de La Laguna, Spain



Numerical methods in radiative transfer

Olga Atanackovic (Email)
Faculty of Mathematics, University of Belgrade, Serbia


Stellar atmosphere codes

Mats Carlsson (Email)
Institute of Theoretical Astrophysics, University of Oslo, Norway


Radiative transfer in the (expanding) atmospheres of early-type stars, and related problems

Jo(achim) Puls (Personal webpage - Email)
Universitaetssternwarte der LMU Munchen, Germany


Phenomenology and physics of late-type stars

Maria Bergemann (Personal webpage - Email)
Max Planck Institute for Astronomy, Heidelberg, Germany


Modeling the atmospheres of brown dwarfs and extrasolar giant planets

Mark S. Marley (Email)
NASA Ames Research Center, Space Science & Astrobiology Division, USA


Near IR high resolution spectroscopy of variable stars

Giuseppe Bono (Email)
Dipartamento di Fisica, Universita' di Roma Tor Vergata, Italy


Tutorials on the application of radiative transfer codes to the cool and hot star domain

Cool stars
Carlos Allende Prieto (Email)
Instituto de Astrofísica de Canarias, Spain

Hot stars
Sergio Simón-Díaz (Personal webpage - Email)
Instituto de Astrofísica de Canarias, Spain