Zobrazeno 1 - 10
of 119
pro vyhledávání: '"I. Vince"'
Autor:
I. Vince
Publikováno v:
Chemical Engineering Transactions, Vol 31 (2013)
A potentially dangerous explosion was triggered by the inadvertent mixing, at ambient temperature, of small quantities of nitric acid and an unidentified organic substance. The explosion occurred in a knock-out vessel at a hazardous waste treatment c
Externí odkaz:
https://doaj.org/article/2330368c9ec04f8cb6295832c445dc4f
Autor:
T. Hegedus, O. Latkovic, H. Markov, I. Vince, A. Cseki, J. Nuspl, N. Markova, E. Rovithis-Livaniou, J. Vinko
Publikováno v:
Odessa Astronomical Publications, Vol 20, Iss 1, Pp 76-77 (2007)
Central-East-South European Binary star study group - CESEB - is an international research team focused on the study of binary stars through combined spectral and photometric observations that can be made using the Bulgarian NAO 2m telescope and seve
Externí odkaz:
https://doaj.org/article/631ac564ff3e435bb8b01571e3c61f1e
Publikováno v:
International Journal of Refrigeration. 131:559-567
Knowledge of sizes of leak holes arising in refrigeration, air conditioning and heat pump systems is critical for safe application of flammable refrigerants, especially hydrocarbons such as R290. Data for leak hole sizes is currently lacking so safet
Publikováno v:
International Journal of Refrigeration. 117:209-217
Currently, industry and governmental entities are increasingly concerned with the restrictive controls on flammable refrigerant – particularly class A3 – charge limits, within safety standards. Since A3 refrigerants, such as R290 and R1270, are i
Autor:
I. Vince, O. Atanackovic
Publikováno v:
Serbian Astronomical Journal, Vol 2020, Iss 201, Pp 49-57 (2020)
We present a short biography and brief review of contributions of professor Mirjana Vukicevic-Karabin to the development of astrophysics education at the University of Belgrade and to the research in physics of the Earth ionosphere and the Sun. The b
Autor:
P. Hadrava, M. Cabezas, G. Djurašević, J. Garcés, S. Y. Gorda, M. I. Jurkovic, D. Korčáková, H. Markov, R. E. Mennickent, J. Petrović, I. Vince, S. Zharikov
Publikováno v:
Astronomy and Astrophysics
Context. The eclipsing close binary UU Cas is an interacting massive double-periodic system with a gainer star partly hidden in an accretion disk. Aims. In order to study the physics of the accretion process in greater detail, along with the structur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::debf314e4e738c0ae4a219a861a0d3df
https://hdl.handle.net/10995/117965
https://hdl.handle.net/10995/117965
Autor:
H. Markov, M. I. Jurkovic, Daniela Korčáková, I. Vince, J. Garcés, Petr Hadrava, Ronald E. Mennickent, M. Cabezas, G. Djurašević, J. Petrović
We present the results of the study of the close binary UU Cassiopeiae based on previously published multi wavelength photometric and spectroscopic data. Based on eclipse timings of the last 117 years, we find an improved orbital period of $\rm P_{o}
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d84310a377d1f1dd1583c3de6a3d911
http://arxiv.org/abs/2009.01352
http://arxiv.org/abs/2009.01352
Autor:
L. Č. Popović, I. Vince
Publikováno v:
Serbian Astronomical Journal, Vol 2018, Iss 196, Pp 29-36 (2018)
Here, we give a short biography and summary of scientific contributions of Aleksandar Kubicela, a doyen of astronomy in Serbia, and an astrophysical research pioneer at the Astronomical Observatory of Belgrade. Additionally, we evoke some of our memo
Publikováno v:
New Astronomy. 15:669-677
The spectral region in the vicinity of 5394 A contains three prominent photospheric spectral lines, which can be used as a solar plasma diagnostic tool. The occurrence of telluric lines in this region is a potential source of systematic and random er
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:329-336
We analyze the CoRoT and V-passband ground-based light curves of the interacting close binary AU Mon, assuming that there is a geometrically and optically thick accretion disk around the hotter and more massive star, as inferred from photometric and