Dec 6, 2016 · Spiral Structure and Differential Dust Size Distribution in the LkH(alpha) 330 Disk Dust trapping accelerates the coagulation of dust particles ...
Combining the results of near-infrared and submillimeter observations, we conjecture that the spiral arms exist at the upper surface and an asymmetric structure ...
Spiral Structure and Differential Dust Size Distribution in the LkH alpha 330 Disk. Mendeley · CSV · RIS · BibTeX ; Date. 2016-12 ; Type. Journal Article.
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 ...
Jul 16, 2016 · SPIRAL STRUCTURE AND DIFFERENTIAL DUST SIZE DISTRIBUTION IN THE LkHα 330 DISK · E. Akiyama, J. Hashimoto, +58 authors. M. Tamura · Published 16 ...
ABSTRACT Dust trapping accelerates the coagulation of dust particles, and, thus, it represents an initial step toward the formation of planetesimals.
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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.
7 days ago · Azimuthal analysis shows that the disk has an asymmetric dust distribution. ... spiral-like structures are highly flared and/or have ...
Dust trapping accelerates the coagulation of dust particles, and thus it represents an initial step toward the formation of planetesimals.
Missing: LkH alpha