1. |
N.
Alonizan, R. Qindeel, N. Ben Nessib, S. Sahal-Br้chot and M. S.
Dimitrijevic
|
Stark
broadening parameters for neutral oxygen spectral lines
|
2. |
A.
Ammar and H. Ghalila
|
Ionoshperic
disturbances due to Solar flares recorded by VLF receiver located in Tunis
|
3. |
K.
Bensch, A. del Olmo and J. Sulentic
|
Measures
of the soft X-ray excess as an eigenvector 1 parameter for Active Galactic
Nuclei
|
4. |
E.
Bon, P. Marziani, J. Sulentic and N. Bon
|
Searching
for a BBH Signature in Quasar Spectra: A 4DE1 Perspective
|
5. |
E.
Danezis, D. Stathopoulos, E. Lyratzi, A. Antoniou and D. Tzimeas
|
From
Quasars to Stars. Similar Phenomena in the Spectra of Quasars and Hot
Emission Stars
|
6. |
M.
S. Dimitrijević, Z. Simić, A. Kovačević and S.
Sahal-Br้chot
|
On
the Stark broadening of Xe VIII spectral lines in White Dwarfs
|
7. |
M.
S. Dimitrijević, Z. Simić, A. Kovačević and S.
Sahal-Br้chot
|
On
the Stark broadening parameters of spectral lines of Neutral Neon
|
8. |
A.
del Olmo, J. Sulentic, P. Marziani, M. A. Martํnez-Carballo and K.
Bensch
|
3C
57, A rejuvenated QSO
|
9. |
R.
V. Munoz-Dimitrova and R. Bachev
|
Spectroscopic
monitoring of AGN at Rozhen observatory
|
10. |
I.
Tapalaga and I. P. Dojčinović
|
Stark
broadening of spectral lines within sodium isoelectronic sequence
|
11. |
M.
Grzedzielski, P. Sukova and A. Janiuk
|
Deterministic
chaos in the X-ray sources
|
12. |
I.
Hannachi, T. Meftah, J. Rosato and R. Stamm
|
Simulation
Calculations of Line Shapes in Presence of Langmuir Turbulence
|
13. |
N.
Ivanović, G. Lj. Majstorović and N. M. iovic
|
The
method for mapping electric field distribution in cathode fall region of
abnormal glow discharge using neutral Neon spectral line shapes
|
14. |
A.
Kolarski and D. Grubor
|
Comparative
analysis of VLF signal variation along trajectory induced by X-ray solar
flares
|
15. |
A.
Kovačević, L. Č. Popović,, A. I. Shapovalova and D. Ilić
|
Exploring
irregular bivariate AGN time series
|
16. |
G.
La Mura, D. Bastieri, M. Berton, G. Chiaro, S. Ciroi, V. Cracco and P.
Rafanelli
|
Properties
of the [OIII] lines in two samples of radio-emitting Seyfert 1 galaxies
|
17. |
E.
Lyratzi, D. Stathopoulos, E. Danezis, A. Antoniou and D. Tzimeas
|
Answers
to some important questions on the use of GR model
|
18. |
Z.
Majlinger, Z. Simić and M. S. Dimitrijević
|
On
the Stark broadening of Lu III spectral lines
|
19. |
A.
A. Mihajlov, N. M. Sakan and V.
A. Srećković
|
The
Inverse bremsstrahlung in astrophysical plasmas: The absorption coefficients
and Gaunt factors
|
20. |
M.
L. Martํnez-Aldama et al.
|
Observations
of the Ca II Ir triplet in high luminosity Quasars: Exploring the sample
|
21. |
C.
A. Negrete, P. Marziani, D. Dultzin and J. W. Sulentic
|
Photoionisation
estimates of broad line region size in high redshift Quasars
|
22. |
A.
Nina, V. M. Čade, J. Bajčetić and M. Andrić
|
Variability
of D-region photoionisation induced by Lyα radiation
|
23. |
R.
Qindeel, N. Alonizan and N. Ben Nessib
|
Atomic
data for transitions in neutral Carbon
|
24. |
S.
Simić and E. Bon
|
Contribution
to SED of AGNs induced by possible density perturbations in complex geometry
of binary systems
|
25. |
M.
Smailagić and E. Bon
|
Modelling
Line Emission from Sub Parsec Spiral Structures around Eccentric Orbits of
Supermassive Binary Black Hole Systems
|
26. |
M.
Smailagić and E. Bon
|
Line
Shapes Emitted from Spiral Structures around Symmetric Orbits of
Supermassive Binary Black Holes
|
27. |
M.
Smailagić
|
Modeling
luminosity and area functions of Lyman-alpha blobs
|
28. |
S.
Vidojević
|
Impulsive
electron events and Langmir waves
|
29. |
J.
Rosato
|
Radiative
transfer reconsidered as quantum kinetic theory problem
|
30. |
Dj.
Savić, L. Č. Popović, R. W. Goosmann and V. L. Afanasiev
|
Theoretical
modeling of polarized broad line profiles of AGN
|
31. |
P.
A. Rojas Lobos and C. M. Gaskell
|
The
production of strong broad He II emission after the tidal disruption of a
main-sequence star by a supermassive black hole
|
32. |
N.
Rakić, G. La Mura, D. Ilić, A.
I. Shapovalova, W. Kollatschny and L.
Č. Popović
|
The
intrinsic Baldwin effect in five long term monitored AGNs
|