Zobrazeno 1 - 10
of 594
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 2009, Iss 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/20313e3aa064443798bd41efd4a1aefd
Publikováno v:
Serbian Astronomical Journal, Vol 2007, Iss 174, Pp 83-88 (2007)
Using the 2-m telescope of the Bulgarian National Astronomical Observatory at Rozhen, observations of 55 multiple stars were carried out during one night, December 16/17. 2006. This is the third series of CCD measurements of double and multiple stars
Externí odkaz:
https://doaj.org/article/0f7904e297474a5993f3df7414343730
Publikováno v:
Serbian Astronomical Journal, Vol 2006, Iss 172, Pp 53-58 (2006)
Using the 2-m telescope of the Bulgarian National Astronomical Observatory at Rozhen observations of twenty multiple stars were carried out during one whole night - October 30/31, and, also, during the first half of the next one - October 31. 2005. T
Externí odkaz:
https://doaj.org/article/a58c38032db94c7f81f833cd49555fcf
Autor:
Novaković B., Todorović N.
Publikováno v:
Serbian Astronomical Journal, Vol 2006, Iss 172, Pp 21-25 (2006)
We present orbits of four double stars. Orbits of stars WDS 23516+4205 = ADS 17050 and WDS 18239+5848 = ADS 11336 were calculated for the first time. Orbits of double stars WDS 02022+3643 = ADS 1613 and WDS 18443+3940 = ADS 11635 were revised. We hav
Externí odkaz:
https://doaj.org/article/a1ef168be25740be8f4dd691bee0a17d
Autor:
Cvetković Z., Novaković B.
Publikováno v:
Serbian Astronomical Journal, Vol 2006, Iss 173, Pp 73-82 (2006)
In this paper orbits for 13 binaries are recalculated and presented. The reason is that recent observations show higher residuals than the corresponding ephemerides calculated by using the orbital elements given in the Sixth Catalog of Orbits of Visu
Externí odkaz:
https://doaj.org/article/3674be7af7d64488ba805bc714bba858
Autor:
Pavlović Rade M., Cvetković Zorica D., Olević Dragomir M., Strigachev A., Popović Georgije M., Novaković B.
Publikováno v:
Serbian Astronomical Journal, Vol 2005, Iss 171, Pp 49-53 (2005)
With the 2-m telescope of the Bulgarian National Astronomical Observatory at Rozhen observations of fifteen multiple stars were carried out during one night - October 17/18, 2004. In the paper we present the results for the position angle and separat
Externí odkaz:
https://doaj.org/article/7d83f91ffc0e42b4ad47790085d1c41e
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