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pro vyhledávání: '"Kostic, Petar"'
We present an analytical model of $\Sigma-D$ relation for supernova remnants (SNRs) evolving in a clumpy medium. The model and its approximations were developed using the hydrodynamic simulations of SNRs in environments of low-density bubbles and clu
Externí odkaz:
http://arxiv.org/abs/2409.07905
Autor:
Wadhwa, Surjit S., Popowicz, Adam, Michel, Raul, Kostic, Petar, Vince, Oliver, Tothill, Nick F. H., De Horta, Ain Y., Filipovic, Miroslav D.
Low mass ratio contact binary systems are more likely to have unstable orbits and potentially merge. In addition, such systems exhibit characteristics such as starspots and high energy emissions (UV) suggestive of chromospheric and magnetic activity.
Externí odkaz:
http://arxiv.org/abs/2407.08365
Autor:
Wadhwa, Surjit S., Landin, Natalia R., Kostic, Petar, Vince, Oliver, Arbutina, Bojan, De Horta, Ain Y., Filipovic, Miroslav D., Tothill, Nicholas F. H., Petrovic, Jelena, Djuravsevic, Gojko
The orbital stability of contact binary systems has been receiving considerable attention recently. Theoretical studies indicate that merger is likely to occur at very low mass ratios, but the actual mass ratio at which merger may take place is likel
Externí odkaz:
http://arxiv.org/abs/2310.06255
Autor:
Prasetya, I. S. W. B., Leek, Craig Q. H. D., Melkonian, Orestis, Tusscher, Joris ten, van Bergen, Jan, Everink, J. M., van der Klis, Thomas, Kostic, Petar, Meijerink, Rick, Oosenbrug, Roan, Oostveen, Jelle J., Pol, Tijmen van den, de Vries, Mike, van Zon, Wink M.
Publikováno v:
Proceedings of 41th ICSE 2019 --- Software Engineering Education and Training (SEET) track, IEEE, 2019
There are many benefits in providing formal specifications for our software. However, teaching students to do this is not always easy as courses on formal methods are often experienced as dry by students. This paper presents a game called FormalZ tha
Externí odkaz:
http://arxiv.org/abs/1903.00334
Akademický článek
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We analyze the influence of fractal structure of the interstellar matter (ISM) density on the parameter values for the radio surface brightness to diameter ($\Sigma-D$) relation for supernovae remnants (SNRs). We model a dense ISM as a molecular clou
Externí odkaz:
http://arxiv.org/abs/1606.02501
Publikováno v:
In Materials Letters 1988 6(11):393-397
