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VII
Serbian Conference on Spectral Line Shapes in Astrophysics
June
15-19, 2009, Zrenjanin, Serbia
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PROGRAM
OF THE CONFERENCE
Sunday,
June 14, 2009
Arrival of participants
Monday,
June 15, 2009
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08:30-09:00
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Registration
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09:00-09:30
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Opening
ceremony
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Chair:
Gillian Peach
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09:30-10:10
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Sylvie
Sahal-Bréchot
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Collisional
line broadening versus collisional atomic depolarization and astrophysical
applications (IL)
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10:10-10:50
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Roland
Stamm
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Spectral
line shapes modeling in laboratory and astrophysical plasmas (IL)
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10:50-11:30
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Martin
Gaskell
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What
spectral line shapes tell us about how AGNs work (IL)
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11:30-12:00
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Coffee
break
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Chair:
Sylvie Sahal-Bréchot
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12:00-12:40
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Maarten
Baes
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A
new view on the ISM of galaxies: far-infrared and submillimetre spectroscopy
with Herschel (IL)
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12:40-13:00
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Darko
Jevremović
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The
project of Serbian virtual observatory
and data for stellar spectra modellisation (PR)
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13:00-15:00
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Lunch
break
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Chair:
Martin Gaskell
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15:00-15:40
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George
Chartas
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High
velocity winds from narrow and broad absorption line quasars (IL)
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15:40-16:00
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Predrag
Jovanović
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Influence
of gravitational microlensing on broad absorption lines of QSOs (PR)
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16:00-16:20
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Alexandrina
A. Smirnova
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Study
of narrow line region in Seyfert galaxy Mrk 1066 (PR)
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16:20-16:40
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Giovanni
La Mura
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Hydrogen
Balmer emission lines and the complex BLR structure (PR)
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16:40-17:10
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Coffee
break
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Chair:
Roland Stamm
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17:10-17:50
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Gillian
Peach
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Spectral
line shapes in cool star (IL)
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17:50-18:10
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Evaggelia
Lyratzi
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Ways
of creation of SACs and DACs in the plasma around quasars (PR)
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18:10-18:30
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Theodoros
Nakos
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Studying
the spectral properties of AGN in the JWST era (PR)
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18:30
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Visiting
the center of Zrenjanin (after that welcome cocktail in the
Municipality
of
Zrenjanin)
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Tuesday, June 16, 2009
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Chair:
Piero Rafanelli
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09:30-10:10
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Jack
Sulentic
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Following
Hβ to
z~3 (IL)
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10:10-10:50
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Milorad
M. Kuraica
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The
connection between spectroscopy of laboratory and astrophysical plasmas (IL)
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10:50-11:20
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Coffee
break
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Chair:
Jack Sulentic
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11:20-12:00
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Emmanouil
Danezis
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Interpretating
the complex line profiles in the stellar spectra (IL)
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12:00-12:40
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Alla
I.
Shapovalova
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Evolution
of the broad emission line profiles in some AGN (IL)
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12:40-13:20
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Derek
Homeier
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Accurate
collisional broadening profiles for alkali resonance lines in substellar
atmosphere models (IL)
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13:20-15:00
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Lunch
break
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Chair:
Michael Eracleous
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15:00-15:40
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Piero
Rafanelli
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Nuclear
activity and star formation properties of Seyfert galaxies (IL)
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15:40-16:20
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Alexei
V. Moiseev
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3D
spectroscopic study of galactic rings: formation and kinematics (IL)
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16:20-16:40
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Dragana
Ilić
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The
line parameters and ratios as a physical probe of the line emitting regions
in AGN (PR)
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16:40-17:00
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Matthias
Zetzl
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QSO/AGN
environments at different redshifts (PR)
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17:00-17:30
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Coffee
break
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Chair:
Emmanouil Danezis
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17:30-18:10
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María
Dolores Calzada Canalejo
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Plasma
of noble gases and their mixtures at atmospheric pressure (IL)
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18:10-18:50
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Magdalena
Christova
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Multiple
perturber effects due to the H-He collisions in the far red wing of Lyα
line (IL)
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Chair:
Nebil Ben Nessib
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18:50-20:00
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Poster
presentations
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Wednesday,
June 17, 2009
Excursion
Thursday,
June 18, 2009
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Chair:
George Chartas
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09:30-10:10
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Michael
Eracleous
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Double-peaked
emission lines as a probe of the broad-line regions of active galactic
nuclei (IL)
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10:10-10:30
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Tamara
Bogdanović
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Emission
lines as a tool in search for supermassive black hole binaries and recoiling
black hole (PR)
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10:30-10:50
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Edi
Bon
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Complex
line profiles of AGN - geometry of the broad line region (PR)
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10:50-11:20
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Coffee
break
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Chair:
María
Dolores Calzada Canalejo
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11:20-12:00
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Andrey
N. Klyucharev
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Rydberg
atoms in astrophysics (IL)
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12:00-12:40
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Damian
J. Christian
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The
search from 6Li in active late-type stars (IL)
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12:40-13:00
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Zoran
Simić
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Stark
broadening spectral lines in chemically peculiar stars (PR)
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13:00-13:20
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Arved-Ervin
Sapar
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Modeling
of mercury isotopes segregation in CP stellar atmospheres: results and
problems (PR)
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13:20-15:00
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Lunch
break
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Chair:
Jagoš Purić
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15:00-15:40
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Anatolij
A. Mihajlov
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The
chemi-ionization processes in the solar photosphere
(IL)
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15:40-18:00
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Poster
presentations (the competition for the best poster)
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19:00
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Conference
dinner
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Friday,
June 19, 2009
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Chair:
John Danziger
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10:30-11:10
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Nebil
Ben Nessib
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Ab
initio calculations of Stark broadening parameters (IL)
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11:10-11:30
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Alexander
Zakharov
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Gravitational
lensing: from micro to nano
(PR)
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11:30-12:00
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Coffee
break
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12:00-12:20
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Closing
ceremony (L. Č. Popović, M. S. Dimitrijević)
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List
of posters
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Maarten
Baes |
The
Variable Star One-shot Project (VSOP): goals, tools, status and science
highlights |
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Nelly
Bonifaci |
Study
of He lines emitted from Corona discharge |
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Viacheslav.
F. Boretskij |
The
role of spectral lines self-absorption in the determinations of the plasma parameters |
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Valentina
Cracco |
Gas
origin in the extended narrow line region of nearby Seyfert galaxies |
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Milan
S. Dimitrijević |
Stark
broadening of Ar XV spectral lines within x-wavelength range |
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Haykel
Elabidi |
Quantum
and semiclassical Stark broadening of 3s-np and nd-5f transitions in C IV, N
V, Mg X and Al XI |
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Rafik
Hamdi |
Ab
initio Stark broadening calculations for Ca V spectral lines |
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Eleni
Kalfountzou |
Spectroscopic
characterization of ULIRG Cirrus |
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Ivan
Y. Katkov |
Stellar
kinematics of AGN host galaxies |
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Evaggelia
Lyratzi |
Studding
the origin of SACs and DACs in the spectra of hot emission stars |
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Walid
F. Mahmoudi |
Semi
classical impact Stark broadening of complex transitions in FeXIV |
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José
Muñoz |
Van
der Waals broadening in atmospheric pressure surface wave discharges
sustained in rare gases |
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Slobodan
Ninković |
Velocity
ellipsoid - Importance of line-of-sight velocities |
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Rodrigo
Parra |
Observations
of sub-millimetre of hydrogen recombinations lines towards etaCarina and
NGC253 |
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Marko
Stalevski |
Line
profile variability due to perturbations in AGN accretion disk emissivity |
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Sonja
Vidojević |
Langmuir
waves statistics and type III bursts observed by wind spacecraft |
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Oliver
Vince |
Dust
attenuation in starburst galaxies |
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Besma
Zmerli |
Stark
broadening calculations of neutral copper
spectral lines
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Legend:
IL
- Invited Lecture (40 min);
PR -
Progress Report (20 min);
P -
Poster (the panel size: 1 x 1.2 m)
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