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Search: WFRF:(Ho Paul T.P.) > (2019)

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1.
  • Akita, Munehira, et al. (author)
  • Asian ergonomics in the new millennium
  • 2000
  • In: Ergonomics for the New Millenium. - : Human Factors and Ergonomics Society. - 0945289138 ; , s. 690-691
  • Conference paper (peer-reviewed)abstract
    • Asia has more than a half of the world population. However, ergonomics has not been widely applied with exceptions of Japan and Korea. Recently, the excitement of ergonomics is being spread to other countries such as Hong Kong, Taiwan, and Indonesia. Although there have been two regional conferences, PPCOE and SEA Conference, Asian ergonomists have not met together to discuss their activities in a world conference. Therefore, the objectives of this symposium is to provide the opportunities for them to discuss the current status of ergonomics and possibly joints efforts to promote ergonomics in Asia. At the same time, this symposium intends to introduce the ergonomics activities in Asia to Western and non-Asian ergonomists and to look for new guidance to enhance its activities from the world renowned exports who have experienced in working in Asia with Asian ergonomists. This syposium consists of two sessions: one panel session and one technical session
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2.
  • Akiyama, E., et al. (author)
  • DISCOVERY OF A DISK GAP CANDIDATE AT 20 AU IN TW HYDRAE
  • 2015
  • In: Astrophysical Journal Letters. - 2041-8205 .- 2041-8213. ; 802:2
  • Journal article (peer-reviewed)abstract
    • We present a new Subaru/HiCIAO high-contrast H-band polarized intensity (PI) image of a nearby transitional disk associated with TW Hydrae. The scattered light from the disk was detected from 0 ''.2 to 1 ''.5 (11-81 AU) and the PI image shows a clear axisymmetric depression in PI at similar to 0 ''.4 (similar to 20 AU) from the central star, similar to the similar to 80 AU gap previously reported from Hubble Space Telescope images. The azimuthal PI profile also shows that the disk beyond 0 ''.2 is almost axisymmetric. We discuss two possible scenarios explaining the origin of the PI depression: (1) a gap structure may exist at similar to 20 AU from the central star because of a shallow slope seen in the PI profile, and (2) grain growth may be occurring in the inner region of the disk. Multi-band observations at near-infrared and millimeter/submillimeter wavelengths play a complementary role in investigating dust opacity and may help reveal the origin of the gap more precisely.
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