Zobrazeno 1 - 10
of 966
pro vyhledávání: '"Lin, P.‐N."'
The origin of planetary mass objects (PMOs) wandering in young star clusters remains enigmatic, especially when they come in pairs. They could represent the lowest-mass object formed via molecular cloud collapse or high-mass planets ejected from thei
Externí odkaz:
http://arxiv.org/abs/2410.21180
Massive stars may form in or be captured into AGN disks. Recent 1D studies employing stellar-evolution codes have demonstrated the potential for rapid growth of such stars through accretion up to a few hundred $M_\odot$. We perform 3D radiation hydro
Externí odkaz:
http://arxiv.org/abs/2408.12017
Star-forming regions, characterized by dense environments, experience frequent encounters that significantly influence binary systems, leading to their hardening, softening, or ionization. We extend the Hut \& Bahcall formalism to derive an analytica
Externí odkaz:
http://arxiv.org/abs/2407.20416
Migration commonly occurs during the epoch of planet formation. For emerging gas giant planets, it proceeds concurrently with their growth through the accretion of gas from their natal protoplanetary disks. Similar migration process should also be ap
Externí odkaz:
http://arxiv.org/abs/2406.12716
Context. About 25% -- 50% of white dwarfs are found to be contaminated by heavy elements, which are believed to originate from external sources such as planetary materials. Elemental abundances suggest that most of the pollutants are rocky objects an
Externí odkaz:
http://arxiv.org/abs/2405.17853
Autor:
Chen, Yi-Xian, Lin, Douglas N. C.
Gravitational instability in the outskirts of Active Galactic Nuclei (AGN) disks lead to disk fragmentation and formation of super-massive (several 10^2Msun) stars with potentially long lifetimes. Alternatively, stars can be captured ex-situ and grow
Externí odkaz:
http://arxiv.org/abs/2404.08780
Autor:
Nayakshin, Sergei, de Miera, Fernando Cruz Saenz, Kospal, Agnes, Calovic, Aleksandra, Eisloffel, Jochen, Lin, Douglas N. C.
In the classical grouping of large magnitude episodic variability of young accreting stars, FUORs outshine their stars by a factor of $\sim$ 100, and can last for up to centuries; EXORs are dimmer, and last months to a year. A disc Hydrogen ionisatio
Externí odkaz:
http://arxiv.org/abs/2403.04439
Dust trapping in the global pressure bump induced by magnetospheric truncation offers a promising formation mechanism for close-in super-Earths/sub-Neptunes. These planets likely form in evolved protoplanetary discs, where the gas temperature at the
Externí odkaz:
http://arxiv.org/abs/2402.14463
Autor:
Wei, Xing, Lin, D. N. C.
We study the magnetic and tidal interactions of a gas-giant exoplanet with its host star and with its exomoons, and focus on their retention. We briefly revisit the scaling law for planetary dynamo in terms of its mass, radius and luminosity. Based o
Externí odkaz:
http://arxiv.org/abs/2402.07387
We perform a series of 3D simulations to study the accretion of giant planet embedded in protoplanetary discs (PPDs) over gap-opening timescales. We find that the accretion mass flux mainly comes from the intermediate latitude above the disc midplane
Externí odkaz:
http://arxiv.org/abs/2310.02822