activity
20032025
most citedIndividual and collective behavior of dust particles in a protoplanetary nebula

70 citations · 146 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025

Tidal disruption and evaporation of rubble-pile and monolithic bodies as a source of flaring activity in Sgr A^\star$

Wen-Han Zhou, Yun Zhang, Jiamu Huang +1

Sgr A*, the supermassive black hole at the center of the Milky Way, exhibits frequent short-duration flares with luminosity greater than 1e34 erg/s across multiple wavelengths. The…

astro-ph.EP2024★ 3 cited

White dwarf magnetospheres: Shielding volatile content of icy objects and implications for volatile pollution scarcity

Wen-Han Zhou, Shang-Fei Liu, Douglas N. C. Lin

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. Element…

astro-ph.EP2014★ 60 cited

Constraining the Oblateness of Kepler Planets

Wei Zhu, Chelsea Huang, George Zhou +1

We use Kepler short cadence light curves to constrain the oblateness of planet candidates in the Kepler sample. The transits of rapidly rotating planets that are deformed in shape…

astro-ph2006

On the Formation of Brown Dwarfs

Ing-Guey Jiang, G. Laughlin, D. N. C. Lin

The observational properties of brown dwarfs pose challenges to the theory of star formation. Because their mass is much smaller than the typical Jeans mass of interstellar clouds,…

astro-ph2003★ 13 cited

On the Formation of Brown Dwarfs

Ing-Guey Jiang, G. Laughlin, D. N. C. Lin

The observational properties of brown dwarfs pose challenges to the theory of star formation. Because their mass is much smaller than the typical Jeans mass of interstellar clouds,…

astro-ph2003★ 70 cited

Individual and collective behavior of dust particles in a protoplanetary nebula

P. Garaud, L. Barrière-Fouchet, D. N. C. Lin

We study the interaction between gas and dust particles in a protoplanetary disk, comparing analytical and numerical results. We first calculate analytically the trajectories of in…