Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Sandor, Zs."'
Publikováno v:
A&A 686, A78 (2024)
The ring-like structures in protoplanetary discs that are observed in the cold dust emission by ALMA, might be explained by dust aggregates trapped aerodynamically in pressure maxima. The effect of a transient pressure maximum is investigated that de
Externí odkaz:
http://arxiv.org/abs/2402.11584
In this paper, we present a large-scale dynamical survey of the trans-Neptunian region, with particular attention to mean-motion resonances (MMRs). We study a set of 4121 trans-Neptunian objects (TNOs), a sample far larger than in previous works. We
Externí odkaz:
http://arxiv.org/abs/2302.01221
Publikováno v:
A&A 657, A135 (2022)
Context. A region at the inner edge of the main asteroid belt is populated by the Hungaria asteroids. Among these objects, the Hungaria family is formed as the result of a catastrophic disruption of (434) Hungaria asteroid hundred million years ago.
Externí odkaz:
http://arxiv.org/abs/2110.11745
Publikováno v:
A&A 642, A140 (2020)
Recent observations of protoplanetary disks have revealed ring-like structures that can be associated to pressure maxima. Pressure maxima are known to be dust collectors and planet migration traps. Most of planet formation works are based either on t
Externí odkaz:
http://arxiv.org/abs/2005.10868
The identification of mean motion resonances in exoplanetary systems or in the Solar System might be cumbersome when several planets and large number of smaller bodies are to be considered. Based on the geometrical meaning of the resonance variable,
Externí odkaz:
http://arxiv.org/abs/1803.07458
Autor:
Guilera, O. M., Sándor, Zs.
Publikováno v:
A&A 604, A10 (2017)
In the classical core-accretion planet formation scenario, rapid inward migration and accretion timescales of kilometer size planetesimals may not favor the formation of massive cores of giant planets before the dissipation of protoplanetary disks. O
Externí odkaz:
http://arxiv.org/abs/1610.01232
Protoplanetary disks dissipate rapidly after the central star forms, on time-scales comparable to those inferred for planet formation. In order to allow the formation of planets, disks must survive the dispersive effects of UV and X-ray photoevaporat
Externí odkaz:
http://arxiv.org/abs/1512.04622
In this paper the migration of a 10 Earth-mass planetary core is investigated at the outer boundary of the dead zone of a protoplanetary disc by means of 2D hydrodynamic simulations done with the graphics processor unit version of the FARGO code. In
Externí odkaz:
http://arxiv.org/abs/1305.5676
Submillimetre images of transition discs are expected to reflect the distribution of the optically thin dust. Former observation of three transition discs LkHa330, SR21N, and HD1353444B at submillimetre wavelengths revealed images which cannot be mod
Externí odkaz:
http://arxiv.org/abs/1109.6177
Star formation occurs via fragmentation of molecular clouds, which means that the majority of stars born are a members of binaries. There is growing evidence that planets might form in circumprimary disks of medium-separation binaries. The tidal forc
Externí odkaz:
http://arxiv.org/abs/1101.1820