Zobrazeno 1 - 10
of 562
pro vyhledávání: '"Novaković, B."'
Autor:
Athanasopoulos, D., Hanuš, J., Avdellidou, C., van Belle, G., Ferrero, A., Bonamico, R., Gazeas, K., Delbo, M., Rivet, J. P., Apostolovska, G., Todorović, N., Novakovic, B., Bebekovska, E. V., Romanyuk, Y., Bolin, B. T., Zhou, W., Agrusa, H.
Publikováno v:
A&A 690, A215 (2024)
The aim of our study is to characterise the spin states of the members of the Athor and Zita collisional families and test whether these members have a spin distribution consistent with a common origin from the break up of their respective family par
Externí odkaz:
http://arxiv.org/abs/2409.03419
Publikováno v:
A&A 672, A39 (2023)
Context. From numerical simulations, it is known that some secular resonances may affect the motion of near-Earth objects (NEOs). However, the specific location of the secular resonance inside the NEO region is not fully known, because the methods pr
Externí odkaz:
http://arxiv.org/abs/2302.08126
Publikováno v:
Serbian Astronomical Journal, Vol 179, Pp 75-86 (2009)
A procedure of gridification of the computation of asteroid proper orbital elements is described. The need to speed up the time consuming computations and make them more efficient is justified by the large increase of observational data expected from
Externí odkaz:
https://doaj.org/article/93f200dfc5e747eb92f2959f08444a32
Publikováno v:
A&A 649, A115 (2021)
Very young asteroid families may record processes that accompanied their formation in the most pristine way. This makes analysis of this special class particularly interesting. We studied the very young Adelaide family in the inner part of the main b
Externí odkaz:
http://arxiv.org/abs/2103.15398
Asteroid families are formed as the result of collisions. Large fragments are ejected with speeds of the order of the escape velocity from the parent body. After the family formation, the fragments' orbits evolve in the space of proper elements becau
Externí odkaz:
http://arxiv.org/abs/1804.00505
Asteroid families are valuable source of information to many asteroid-related re- searches, assuming a reliable list of their members could be obtained. However, as the number of known asteroids increases fast it becomes more and more difficult to ob
Externí odkaz:
http://arxiv.org/abs/1705.09226
The Hoffmeister family is a C-type group located in the central main belt. Dynamically, it is important because of its interaction with the ${\nu}_{1C}$ nodal secular resonance with Ceres, that significantly increases the dispersion in inclination of
Externí odkaz:
http://arxiv.org/abs/1611.06176
In this work we have estimated 10 collisional ages of 9 families for which for different reasons our previous attempts failed. In general, these are difficult cases that required dedicated effort, such as a new family classifications for asteroids in
Externí odkaz:
http://arxiv.org/abs/1607.01998
Publikováno v:
Therapeutics and Clinical Risk Management, Vol Volume 17, Pp 183-192 (2021)
Barbara Jezeršek Novaković, Lučka Boltežar, Aleksander NovakovićDivision of Medical Oncology, Institute of Oncology Ljubljana, Ljubljana, 1000, SloveniaCorrespondence: Barbara Jezeršek NovakovićDivision of Medical Oncology, Institute of Oncolo
Externí odkaz:
https://doaj.org/article/a7a07d97bfa349708902b90ce5f124bc
Autor:
Knezevic, I., Novakovic, B.
Publikováno v:
J. Comput. Electron. 12, 363 (2013)
Electrons in the active region of a nanostructure constitute an open many-body quantum system, interacting with contacts, phonons, and photons. We review the basic premises of the open system theory, focusing on the common approximations that lead to
Externí odkaz:
http://arxiv.org/abs/1405.4963