Department of Astronomy


Faculty of Mathematics


University of Belgrade

dr Bojan Arbutina

Assistant Professor


Address: Studentski trg 16
               11000 Belgrade
               Serbia
Office: 809, V floor
Phone: +381 11 2027 827
E-mail: arbo@matf.bg.ac.rs



Courses:

Bibliography


See CURRICULUM VITAE (in Serbian).

Selected papers:


B. Arbutina, D. Urošević, M. Stanković, Lj. Tešić:
L-D DEPENDENCE FOR SUPERNOVA REMNANTS AND ITS CONNECTION WITH THE Σ - D RELATION,
2004, Mon. Not. R. Astron. Soc., 350, 346
B. Arbutina, D. Urošević:
Σ - D RELATION FOR SUPERNOVA REMNANTS AND ITS DEPENDENCE ON THE DENSITY OF THE INTERSTELLAR MEDIUM,
2005, Mon. Not. R. Astron. Soc., 360, 76
B. Vukotić, B. Arbutina, D. Urošević:
ON THE MAGNETIC FIELD EVOLUTION IN SHELL-LIKE SUPERNOVA REMNANTS,
2007, Rev. Mex. Astron. Astrophys., 43, 33
B. Arbutina:
CONSTRAINTS ON THE MASSIVE SUPERNOVA PROGENITORS,
2007, International Journal of Modern Physics D, 10 (7), 1219
B. Arbutina:
THE MINIMUM MASS RATIO OF W UMA-TYPE BINARY SYSTEMS,
2007, Mon. Not. R. Astron. Soc., 377, 1635
D. Onić, B. Arbutina, D. Urošević:
RADIAL DEPENDENCE OF EXTINCTION IN PARENT GALAXIES OF SUPERNOVAE,
2008, Rev. Mex. Astron. Astrophys., 44, 103
B. Arbutina:
POSSIBLE SOLUTION TO THE PROBLEM OF THE EXTREME MASS RATIO W UMA-TYPE BINARIES,
2009, Mon. Not. R. Astron. Soc., 394, 501
B. Arbutina, D. Urošević, M. M. Andjelić, M. Z. Pavlović, B. Vukotić:
MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS,
2012, Astrophys. J., 746, 79
D. Onić, D. Urošević, B. Arbutina, D. Leahy:
ON THE EXISTENCE OF "RADIO THERMALLY ACTIVE" GALACTIC SUPERNOVA REMNANTS,
2012, Astrophys. J., 756, 61
M. Z. Pavlović, D. Urošević, B. Vukotić, B. Arbutina, Ü. D. Göker:
THE RADIO SURFACE-BRIGHTNESS-TO-DIAMETER RELATION FOR GALACTIC SUPERNOVA REMNANTS: SAMPLE SELECTION AND ROBUST ANALYSIS WITH VARIOUS FITTING OFFSETS,
2013, Astrophys. J. Suppl. Series, 204, 4
B. Arbutina, D. Urošević, M. M. Vučetić, M. Z. Pavlović, B. Vukotić:
MODIFIED EQUIPARTITION CALCULATION FOR SUPERNOVA REMNANTS. CASES α=0.5 AND α=1,
2013, Astrophys. J., 777, 31

Biography


Bojan Arbutina was born in Belgrade in 1977. He received his primary and secondary education in Slatina and Glina, in Croatia, and in Belgrade. For two years he was enrolled in a study program at the Faculty of Civil Engineering in Belgrade, after which, in 1998/99 he decides to study Astrophysics at the Faculty of Mathematics. He graduated in 2003, and continued postgraduate studies in 2004/05 godine, after the army service. At the same time he was employed as a young research assistant at the Astronomical Observatory of Belgrade. He was awarded M.Sc. degree on December 26 2005, for his thesis entitled "Importance of Supernova Type for the Hydrodynamic and Radio Evolution of Its Remnant". In 2006/07 he became a teaching assistant at the Department of Astronomy, Faculty of Mathematics, University of Belgrade. He obtained his Ph.D. at the same university on June 26 2009, for disseration "The minimum mass ratio for contact close binary systems of W Ursae Majoris-type". His main fields of research are supernovae, hydrodinamic and radio evolution of supernova remnants, and dynamical evolution and stability of close binary systems. He published several paper (see CV). From 2005 he is assistant editor of the Serbian Astronomical Journal and administrator for the Publications of the Astronomical Observatory of Belgrade web site.


Links


Web pages:


http://www.aob.bg.ac.rs/~barbutina/
http://alas.matf.bg.ac.rs/~af98003/
http://solair.EUnet.rs/~arbo/