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researcher

H. Shang

89 papers hereh-index 415.6k citations131 works total

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

author position
  • sole author1
  • first author2
  • middle author57
  • last author20

Across the 80 of 89 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR39
  • astro-ph.GA28
  • astro-ph14
  • astro-ph.EP5
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • H. Shang — 37 papers, h 23
  • H. Shang — 27 papers, h 5
  • H. Shang — 13 papers, h 4
  • H. Shang — 9 papers, h 5
  • H. Shang — 4 papers, h 3
  • H. Shang — 3 papers, h 1

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

activity
20012026
most citedBright X-ray flares in Orion young stars from COUP: evidence for star-disk magnetic fields?

284 citations · 4k across the 88 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.SR2015★ 8 cited

A Two-Temperature Model of Magnetized Protostellar Outflows

Liang-Yao Wang, Hsien Shang, Ruben Krasnopolsky +1

We explore kinematics and morphologies of molecular outflows driven by young protostars using magnetohydrodynamic simulations in the context of the unified wind model of Shang et a…

astro-ph.IM2015★ 8 cited

A Hydrochemical Hybrid Code for Astrophysical Problems. I. Code Verification and Benchmarks for Photon-Dominated Region (PDR)

Kazutaka Motoyama, Oscar Morata, Hsien Shang +2

A two dimensional hydrochemical hybrid code, KM2, is constructed to deal with astrophysical problems that would require coupled hydrodynamical and chemical evolution. The code assu…

astro-ph.GA2015★ 69 cited

Jet Motion, Internal Working Surfaces, and Nested Shells in the Protostellar System HH 212

Chin-Fei Lee, Naomi Hirano, Qizhou Zhang +3

HH 212 is a nearby (400 pc) highly collimated protostellar jet powered by a Class 0 source in Orion. We have mapped the inner 80" (~ 0.16 pc) of the jet in SiO (J=8-7) and CO (J=3-…

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