1. Research with MATF

Arbutina, Bojan

Network Lab View Statistics Email Alert RSS Feed

Profile

Full Name
Arbutina, Bojan
Variants
Arbutina, B.
 
Main Affiliation
 
ORCID
 
Scopus Author ID
Loading... 2 0 20 0 false
Loading... 3 0 20 0 false

Publications

Results 21-40 of 47 (Search time: 0.001 seconds).

Issue DateTitleAuthor(s)Rank
2129-Apr-2015Blast waves with cosmic raysArbutina, Bojan 
221-Jan-2015Optical supernova remnants in nearby galaxies and their influence on star formation rates derived from Hα emissionVučetić, M. M.; Arbutina, Bojan ; Urošević, Dejan 
231-Jan-2014The H-R diagram for supernova remnantsArbutina, Bojan 
241-Jan-2014On calibration of some distance scales in astrophysicsVukotić, B.; Jurković, M.; Urošević, Dejan ; Arbutina, Bojan 
2527-Dec-2013Optical observations of the nearby galaxy IC342 with narrow band [SII] and Hα filters. IVučetić, M. M.; Arbutina, Bojan ; Urošević, Dejan ; Dobardžić, A.; Pavlović, M. Z.; Pannuti, T. G.; Petrov, N.
2620-Nov-2013Relativistic non-thermal bremsstrahlung radiationZeković, Vladimir ; Arbutina, Bojan ; Dobardžić, Aleksandra; Pavlović, Marko Z.
271-Nov-2013Modified equipartition calculation for supernova remnants. Cases α = 0.5 and α = 1Arbutina, Bojan ; Urošević, Dejan ; Vučetić, M. M.; Pavlović, M. Z.; Vukotić, B.
2823-Sep-2013Citation of the Serbian astronomical journal in the period 2010-2012Arbutina, Bojan 
291-Jan-2013The radio surface-brightness-to-diameter relation for galactic supernova remnants: Sample selection and robust analysis with various fitting offsetsPavlović, M. Z.; Urošević, Dejan ; Vukotić, B.; Arbutina, Bojan ; Göker, Ü D.
303-Aug-2012Instructions for authorsArbutina, Bojan ; Urošević, Dejan ; Knežević, Z.
3110-Feb-2012Modified equipartition calculation for supernova remnantsArbutina, Bojan ; Urošević, Dejan ; Andjelić, M. M.; Pavlović, M. Z.; Vukotić, B.
321-Jan-2012On the existence of "radio thermally active" Galactic supernova remnantsOnić, D.; Urošević, Dejan ; Arbutina, Bojan ; Leahy, D.
331-Jan-2011Numerical code for fitting radial emission profile of a shell supernova remnant. ApplicationOpsenica, S.; Arbutina, Bojan 
341-Jan-2011Maximum mass ratio of am CVn-type binary systems and maximum white dwarf mass in ultra-compact X-ray binariesArbutina, Bojan 
358-Oct-2010The orthogonal fitting procedure for determination of the empirical ∑-D relations for supernova remnants: Application to starburst galaxy M82Urošević, Dejan ; Vukotić, B.; Arbutina, Bojan ; Sarevska, M.
361-Dec-2009Optical observations of M81 galaxy group in narrow band [SII] and Hα filters: Holmberg IXArbutina, Bojan ; Ilić, Dragana ; Stavrev, K.; Urošević, Dejan ; Vukotić, B.; Onić, D.
371-Sep-2009The minimum mass ratio for contact close binary systems of W Ursae Majoris-typeArbutina, Bojan 
381-Feb-2009The ∑ - D relation for planetary nebulaeUrošević, Dejan ; Vukotić, B.; Arbutina, Bojan ; Ilić, Dragana ; Filipović, M.; Bojičić, I.; Šegan, S.; Vidojević, S.
391-Jan-2009Possible solution to the problem of the extreme mass ratio W UMa-type binariesArbutina, Bojan 
401-Apr-2008Radial dependence of extinction in parent galaxies of supernovaeOnić, D.; Arbutina, Bojan ; Urošević, Dejan