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W. Thi

35 papers hereh-index 10590 citations24 works total

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

author position
  • first author5
  • middle author24
  • last author2

Across the 31 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA11
  • astro-ph.SR9
  • astro-ph7
  • astro-ph.EP4
  • astro-ph.IM2
  • gr-qc2
same name
  • W. Thi — 99 papers, h 42

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 citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.8k across the 35 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 24 cited

Signatures of warm carbon monoxide in protoplanetary discs observed with Herschel SPIRE

M. H. D. van der Wiel, D. A. Naylor, I. Kamp +9

Molecular gas constitutes the dominant mass component of protoplanetary discs. To date, these sources have not been studied comprehensively at the longest far-infrared and shortest…

astro-ph.GA2014★ 16 cited

A common column density threshold for scattering at 3.6 mum and water-ice in molecular clouds

M. Andersen, W-F. Thi, J. Steinacker +1

Context: Observations of scattered light in the 1-5 μm range have revealed dust grains in molecular cores with sizes larger than commonly inferred for the diffuse interstellar me…

astro-ph.GA2014★ 20 cited

Detecting scattered light from low-mass molecular cores at 3.6 μm - Impact of global effects on the observation of coreshine

J. Steinacker, M. Andersen, W. -F. Thi +1

Recently discovered scattered light at 3-5 μm from low-mass cores (so-called "coreshine") reveals the presence of grains around 1 μm, which is larger than the grains found in t…

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