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Hsiang-Hsu Wang

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP1
  • astro-ph.GA1
  • astro-ph.IM1
ORCID 0000-0001-8436-8803
same name
  • Hsiang-Hsu Wang — 2 papers, h 8

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedFormation of Isothermal Disks around Protoplanets. I. Introductory Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets

18 citations · 26 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.IM2019★ 2 cited

Self-gravitational Force Calculation of High-Order Accuracy for Infinitesimally Thin Gaseous Disks

Hsiang-Hsu Wang, Ming-Cheng Shiue, Rui-Zhu Wu +1

Self-gravitational force calculation for infinitesimally thin disks is important for studies on the evolution of galactic and protoplanetary disks. Although high-order methods have…

astro-ph.GA2014★ 6 cited

Spiral Density Waves in M81. II. Hydrodynamic Simulations for Gas Response to Stellar Spiral Density Waves

Hsiang-Hsu Wang, Wing-Kit Lee, Ronald E. Taam +2

Gas response to the underlying stellar spirals is explored for M81 using unmagnetized hydrodynamic simulations. Constrained within the uncertainty of observations, 18 simulations a…

astro-ph.EP2014★ 18 cited

Formation of Isothermal Disks around Protoplanets. I. Introductory Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets

Hsiang-Hsu Wang, Defu Bu, Hsien Shang +1

The regular satellites found around Neptune ($\approx 17~M_{\Earth}$) and Uranus ($\approx 14.5~M_{\Earth}$) suggest that past gaseous circumplanetary disks may have co-existed wit…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.