Objavljeni radovi:
[1]
1. Kostić, P., Vukotić, B., Urošević, D., Arbutina, B., Prodanović, T., 2016: “Interstellar medium structure and the slope of the radio Ʃ–D relation of supernova remnants”, Mon. Not. R. Astron. Soc., 461, 1421- 1430, IF(2016): 4.961, https://doi.org/10.1093/mnras/stw1381
[2]
1. Kostić, P., 2019: “A new numerical code for hydrodynamical 3D simulations of supernova remnants”, Serbian Astronomical Journal, 199, 65-82, IF(2019): 0.565, https://doi.org/10.2298/SAJ1999065K 2. Kostić, P., Knežević, S., Vukotić, B., 2019: “Hydrodynamics of supernova remnants: interaction with interstellar medium”, Observing techniques, instrumentation and science for metre-class telescopes II, Tatranská Lomnica, Slovakia, September 24-28, 2018, Contrib. Astron. Obs. Skalnate Pleso, 49, 377- 379, IF(2019): 0.636, ISSN: 1336–0337 Саопштења са међународног скупа штампана у изводу (М34): 1. Kostić, P., 2022: “Synchrotron Emission of SNRs in Clumpy Medium”, 3D Supernova (Remnants). How to connect simulations and observations?, Valencia, Spain, September 5-8, 2022 2. Kostić, P., Arbutina, B., Vukotić, B., Urošević, D., 2022: “Synchrotron Emission of SNRs in Clumpy Medium”, Supernova Remnants and their Progenitors, Hybrid (hosted virtually and at the Center for Astrophysics, Harvard & Smithsonian), USA, August 16-18, 2022 3. Kostić, P., 2019: “3D hydrodynamical simulation of the clumpy supernova ejecta”, Anisotropies in core-collapse supernova explosions, Palermo, Italy, October 21-23, 2019 4. Kostić, P., Vukotić, B., 2019: “Hydrodynamical simulations of supernova remnant in fractal interstellar medium: morphology of the shock-wave”, Supernova Remnants II: An Odyssey in Space after Stellar death, Chania, Grece, June 3-8, 2019, Abstract book, p. 71.
