273 citations · 3.9k across the 82 of their papers we have counts for
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The JCMT BISTRO Survey: An 850/450m Polarization Study of NGC 2071IR in OrionB
A-Ran Lyo, Jongsoo Kim, Sarah Sadavoy +143
We present the results of simultaneous 450 m and 850 m polarization observations toward the massive star forming region NGC 2071IR, a target of the BISTRO (B-fields in Star-F…
Impact of Differential Dust Settling on the SED and Polarization: Application to the Inner Region of the HL Tau Disk
Takahiro Ueda, Akimasa Kataoka, Shangjia Zhang +3
The polarimetric observations on the protoplanetary disk around HL Tau have shown the scattering-induced polarization at ALMA Band 7, which indicates that the maximum dust size is…
Estimate on dust scale height from ALMA dust continuum image of the HD 163296 protoplanetary disk
Kiyoaki Doi, Akimasa Kataoka
We aim at estimating the dust scale height of protoplanetary disks from millimeter continuum observations. First, we present a general expression of intensity of a ring in a protop…
Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry
Chakali Eswaraiah, Di Li, Ray S. Furuya +142
We have obtained sensitive dust continuum polarization observations at 850 m in the B213 region of Taurus using POL-2 on SCUBA-2 at the James Clerk Maxwell Telescope (JCMT), as…
The CO core mass function toward Orion A: Single-dish observations
Hideaki Takemura, Fumitaka Nakamura, Shun Ishii +6
We have performed an unbiased dense core survey toward the Orion A Giant Molecular Cloud in the CO (=1--0) emission line taken with the Nobeyama Radio Observatory (NRO) 4…
ALMA observation of the protoplanetary disk around WW Cha: faint double-peaked ring and asymmetric structure
Kazuhiro D. Kanagawa, Jun Hashimoto, Takayuki Muto +13
We present Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations of dust continuum emission of the disk around WW Cha. The dust continuum image shows a smooth dis…
Rotational Disruption of Porous Dust Aggregates due to Gas Flow in Protoplanetary Disks
Misako Tatsuuma, Akimasa Kataoka
We introduce a possible disruption mechanism of dust grains in planet formation by their spinning motion. This mechanism has been discussed as rotational disruption for the interst…