Poster session

. Posters list and abstracts:

1. Non conservative Rayleigh scattering. A perturbative approach,
H. Frisch, pdf

2. Early B-type stars with resolved Zeeman split lines,
S. Hubrig, pdf

3. Radiation effects on impact of accretion streams in Classical T - Tauri Stars,
S. Colombo, pdf

4. Methods to solve multi-dimensional polarized radiative transfer equation with line scattering, magnetic fields and partial frequency redistribution,
A. Lokanathapura Seetharamabhasari, pdf

5. A spectroscopic and kinematical analysis of the hottest white dwarfs from the SDSS DR14,
N. Reindl, pdf

6. Effects of angle-dependent partial frequency redistribution on polarized line profiles,
S. Malali, pdf

7. Polarized line formation with Paschen-Back effect and partial frequency redistribution,
S. Malali,  pdf

8. The Quasi-WR stars HD 45166 and WR 7a revisited,
B. Doležalová, pdf

9. Spectroscopic features of an evolved hot chemically peculiar star: HR 62 (B8 III),
T. Kılıçoğlu, pdf

10. Atmospheric parameters and chemical abundances of pulsating Beta Cephei stars in open clusters,
E. Niemczura, pdf

11. MontAGN - A 3D Radiative Transfer Code for the Modelling of Active Galactic Nuclei and Super Star Clusters,
T. Nguyen, pdf

12. A new near-IR C2 linelist for improved chemical analysis of hydrogen deficient carbon-rich giants,
D. Garcia-Hernandez, pdf

13. Astroserver Live - Online spectral analysis with Tlusty models,
P. Nemeth, pdf

14. 3D Monte Carlo Radiative Transfer in inhomogeneous massive star winds : application to resonance line formation,
B. Kubátová, pdf

15. maKe Atoms Simple (KAS): a tool for create, manipulate and build model atoms,
Y. Osorio, pdf

16. Thermally driven disk winds in X-ray binaries - radiation-hydrodynamic simulations,
N. Higginbottom, pdf

17. Python - a Monte Carlo radiative transfer and ionization code,
N. Higginbottom, pdf

18. Radial Abundance gradients of OB stars in the outer Galactic disk,
S. Daflon. pdf

19.The formation of strong emission lines in stellar accretion disks: The link between observations and models,
B. Tessore, pdf

Instructions for Poster Sessions:

The poster boards provided are metallic (grid) vertical rectangles.
We recommend a standard A0 (841x1189mm)  or A1 (594 x 814 mm) formats, portrait size.
They will be attached with magnets of the boards.

 
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