Zobrazeno 1 - 10
of 533
pro vyhledávání: '"Ozernoy, A."'
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 15 July 2020 475:71-76
Autor:
Logunov, Dmitri V.1 Dmitry.Logunov@zin.ru, Ozernoy, Anatoly V.2 pauk.t64@gmail.com
Publikováno v:
Arachnology. 2022, Vol. 19 Issue 3, p635-644. 10p.
Autor:
Ozernoy, Anatoly V. pauk.t64@gmail.com, Logunov, Dmitri V.1 dmitri.v.logunov@manchester.ac.uk
Publikováno v:
Newsletter of the British Arachnological Society. Spring2023, Issue 156, p7-10. 4p.
Autor:
Ipatov, Sergei I., Ozernoy, Leonid M.
Trans-Neptunian objects (TNOs) with diameter greater than 100 km currently moving in not too eccentric orbits could be formed directly by the contraction of large rarefied condensations. Along with the gravitational influence of planets, gravitationa
Externí odkaz:
http://arxiv.org/abs/astro-ph/0107591
Our efficient numerical approach has been applied to modeling the asymmetric circumstellar dust disk around Beta Pictoris as observed with the HST/STIS. We present a new model on the origin of the warping of the Beta Pic disk. We suggest that the obs
Externí odkaz:
http://arxiv.org/abs/astro-ph/0012470
Autor:
Ozernoy, Leonid M.
(abridged) This review is based on an extensive work done in collaboration with N. Gorkavyi, J. Mather, and T. Taidakova, which aimed at the physical modelling of the interplanetary dust (IPD) cloud in the Solar system, i.e., establishing a link betw
Externí odkaz:
http://arxiv.org/abs/astro-ph/0012033
Our numerical simulations of the Edgeworth-Kuiper belt objects gravitationally scattered by the four giant planets accounting for mean motion resonances reveal numerous resonant gaps in the distribution of the scattered population.
Comment: 2 pa
Comment: 2 pa
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010402
We apply our recently elaborated, powerful numerical approach to the high-resolution modeling of the structure and emission of circumstellar dust disks, incorporating all relevant physical processes. Specifically, we examine the resonant structure of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0007014
(Abridged) Using an efficient computational approach, we have reconstructed the structure of the dust cloud in the Solar system between 0.5 and 100 AU produced by the Kuiper belt objects. Our simulations offer a 3-D physical model of the `kuiperoidal
Externí odkaz:
http://arxiv.org/abs/astro-ph/0006435
We have applied a powerful numerical approach to compute, with a high resolution, the structure of dusty circumstellar disks with embedded planets. We emphasize some testable implications of our simulations which would verify the presence of a planet
Externí odkaz:
http://arxiv.org/abs/astro-ph/0005347