VI Serbian Conference on Spectral Line Shapes in Astrophysics
Sremski Karlovci, Serbia June 11-15 2007

This conference is a part of the activities on the occasion of the 120th anniversary of Astronomical Observatory of Belgrade

 

List of Participants


No Name Surname Country Contribution Institution
1 Bojan Arbutina Serbia Radial dependence of extinction in parent galaxies
of supernovae (P)
Astronomical Observatory Belgrade
2 Paul Barklem Sweden The broadening of spectral lines by collisions with
neutral hydrogen atoms in cool stars (IL)
Uppsala University
3 Nebil Ben Nessib Tunisa Experimental and theoretical  determination of
temperature in plasmas (IL)
Faculté des Sciences de Bizerte, Tunisia
4 Edi Bon Serbia The Broad Ha and Hb emission line shapes in
an AGN sample (ST)
Astronomical Observatory Belgrade
5 Viacheslav F.  Boretskij Ukraine Shapes of spectral lines of nonuniform plasma of electric arc discharge between copper electrodes (ST) Radiophysics Dept. Taras Schevchenko Kyiv National University
6 George Chartas USA Absorption Line Diagnostics of Quasar Outflows (IL) Penn State University
7 Eleni Chatzichristou Greece  Studding the complex absorption and emission
lines in AGNs spectra (ST)
Institute of Astronomy and Astrophysics, National Observatory of Athens
8 Magdalena Christova Bulgaria On the broadening of spectral lines in surface
waves sustained discharges (IL)
Technical University-Sofia
9 Miodrag Dacic Serbia Stark broadening of Cr II spectral lines in
stellar atmospheres
Astronomical Observatory Belgrade
10 Emmanouel Danezis Greece The DACs and SACs effects from stars to Quasars.
Some first general notices (IL)
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and Mechanics 
11 John Danziger Italy Profiles in Novae Spectra (IL) Astronomical Observatory Trieste
12 Milan Dimitrijevic Serbia Stark broadening of Cr II spectral lines in
stellar atmospheres (ST)
Astronomical Observatory Belgrade
13 Natasa Gavrilovic Serbia Connection between central black hole and
circum-nuclear gas kinematics: The case of AGN
with double-peaked lines (P)
Astronomical Observatory Belgrade
14 Derek Homeier Germany Collisional Broadening of Na I in Metal-rich White Dwarfs - Beyond the Single Perturber Approximation (ST) Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen
15 Dragana Ilic Serbia Physical properties of the BLR:
Boltzmann-Plot vs. CLOUDY calculations (ST)
Department of Astronomy, Faculty of Mathematics, University of Belgrade
16 Zeljko Ivezic USA SDSS Spectroscopic Survey(s) (IL) University of Washington
17 Darko Jevremovic Serbia The influence of Chemi-Ionization and Chemi-Recombination Processes on H lines in M Dwarf Atmospheres(P) Astronomical Observatory Belgrade
18 Predrag Jovanovic Serbia The shape of the Fe Ka spectral line in the case
of partly obscured accretion disk (ST)
Astronomical Observatory Belgrade
19 Andrei N. Klyucharev Russia Chemi-ionization processes. Alkali-metal
geocosmical plasmas (IL)
St Petersburg State University / Research Institute of Physics
20 Wolfram Kollatschny Germany Line Profile Variability in AGNs (IL) Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen
21 Jelena Kovacevic Serbia Asymmetry of the CIV 1549 line in a sample of
RQ and RL AGN (P)
Astronomical Observatory Belgrade
22 Andjelka Kovacevic Serbia Lag Between the Optical Continuum and
Line Variabilities of NGC 4151 (P)
Department of Astronomy, Faculty of Mathematics, University of Belgrade
23 Giovanni La Mura Italy Detailed analysis of Balmer Lines in a selected
sample of 90 broad line AGN (ST)
Dipartimento di Astronomia, Universita di Padova
24 Evaggelia  Lyratzi Greece The evolution of some physical parameters in the DACs/SACs regions in Be stellar atmospheres (ST) University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and Mechanics 
25 Anatolij A. Mihailov Serbia The influence of ion-atom and atom-Rydberg
atom processes to the continuous and line spectra
of star's atmospheres (P)
Institute of physics
26 Zarko Mijajlovic Serbia Stellar Spectroscopy on the New Astronomical Station
at the Mountain Vidojevica (P)
Faculty of Mathematics, University of Belgrade
27 Nenad Milovanovic Serbia Cowan Code and Stark Broadening of Spectral Lines of S II, S III and S IV (ST) Astronomical Observatory Belgrade
28 Alexei Moiseev Russia The jet-clouds interaction in AGN: a panoramic spectroscopy view (IL) Special Astrophysical Observatory of RAS
29 Slobodan  Ninkovic Serbia Studies of Local Milky-Way Kinematics via
Line-of-Sight Velocities (IL)
Astronomical Observatory Belgrade
30 Gillian  Peach UK Recent work on line shapes for
the spectra of cool stars  (IL)
Department of Physics and Astronomy, University College London
31 Nada Pejovic Serbia Stellar Spectroscopy on the New Astronomical Station
at the Mountain Vidojevica (P)
Department of Astronomy, Faculty of Mathematics, University of Belgrade
32 Zoran Petrovic Serbia Electron, ion and atom collisions leading
to anomalous Doppler broadening in hydrogen
and hydrogen rare gas mixtures (IL)
Institute of physics
33 Luka Popovic Serbia   Astronomical Observatory Belgrade
34 Philippe Prugniel France Modeling the spectrum of the stellar population
in star forming and active galaxies (IL)
CRAL-Observatoire de Lyon
35 Jagos Puric Serbia Stark parameters regularities of multiply charged
ions spectral lines originating from the same
transition array (IL)
Faculty of Physics, University of Belgrade
36 Piero Rafanelli Italy 3D spectroscopy of nuclear and extranuclear
regions of nearby AGN (IL)
Dipartimento di Astronomia, Universita di Padova
37 Mikhail Sachkov Russia Pulsation tomography of roAp stars (IL) Institute of astronomy RAS
38 Nenad Sakan Serbia The modeling of the continuous emission spectrum of a dense non-ideal plasma in optical region (ST) Institute of physics
39 Zoran Simic Serbia Experimental and theoretical stark widths for Au II (P) Astronomical Observatory Belgrade
40 Sasa Simic Serbia Spectral lines in the afterglow of Gamma Ray Bursts (ST) University of Kragujevac, Faculty of Science, Department of Physics
41 Aleksandrina Smirnova Russia Mrk334: connection between nuclei activity and
merging of a companion (ST)
Special Astrophysical Observatory of RAS
42 Vladimir Sreckovic Serbia The modeling of the continuous emission spectrum of a dense non-ideal plasma in optical region (ST) Institute of physics
43 Ilija Stefanovic Germany Plasma analogue for astrophysical dust (IL) Institute for Experimental Physics II, Ruhr University Bochum
44 Paolo Tozzi Italy Emission lines in X--ray spectra of
Clusters of Galaxies (IL)
INAF Osservatorio Astronomico di Trieste
45 Dejan Urosevic Serbia Optical search for supernova remnants in
M81, M82 and NGC 3077 (P)
Department of Astronomy, Faculty of Mathematics, University of Belgrade
46 Sonja  Vidojevic Serbia

Correlation Line-of-Sight Velocity-Metallicity in a Sample of Stars with Possible Planetary Systems (ST)
 An Analysis of Local Milky-Way Kinematics based on Proper-Motion and Line-of-Sight-Velocity Data (P)

Department of Astronomy, Faculty of Mathematics, University of Belgrade
47 Branislav Vukotic Serbia Optical search for supernova remnants in
M81, M82 and NGC 3077 (P)
Astronomical Observatory Belgrade
48 Alexander Zakharov Russia The Fe K-alpha line simulations for BHs:
the simplest model (IL)
State Scientific Center - Institute of Theoretical and Experimental Physics

 

 

 

 

 

 

 

 

 

 

 

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