Dec 6, 2016 · Spiral Structure and Differential Dust Size Distribution in the LkH(alpha) 330 Disk Dust trapping accelerates the coagulation of dust particles ...
Dust trapping accelerates the coagulation of dust particles, and thus it represents an initial step toward the formation of planetesimals.
Spiral Structure and Differential Dust Size Distribution in the LkH alpha 330 Disk ... Planetary systems; Stars: pre-main sequence; Stars: individual (LkH alpha ...
LkH α 𝛼 \alpha 330 was observed at 343.796 GHz, corresponding to 0.87 mm in wavelength, by the SMA on December 18th 2014 (UT). The very extended configuration ...
We discuss the origin of the spiral arm and the asymmetric structure, and suggest that a massive unseen planet is the most plausible explanation. [2]. The ...
Missing: LkH alpha
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Missing: LkH alpha
In this paper, we present new scattered light and millimeter observations of the protoplanetary disk around LkHα 330, using SPHERE/VLT and ALMA, respectively.
SPIRAL STRUCTURE AND DIFFERENTIAL DUST SIZE DISTRIBUTION IN THE LkH alpha 330 DISKDOI Akiyama, E ; Hashimoto, J ; Liu, HB ; Li, JIH ; Bonnefoy, M ; Dong, ...
Spiral Structure of M83-Distribution and ... Spiral structure of M51-Distribution ... Differential Dust Size Distribution in the LKH\ensuremath{alpha} 330 Disk.
Jul 25, 2022 · In addition, the outer spiral arm launched by the planet changes its pitch angle along the spiral due to the eccentricity and when it interacts ...