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researcher

T. L. S. Wong

19 papers hereh-index 6121 citations18 works total

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

author position
  • first author7
  • middle author7
  • last author4

Across the 18 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR17
  • astro-ph.GA1
  • astro-ph.HE1

identity via Semantic Scholar / OpenAlex

activity
20192026
most citedImproved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3

74 citations · 155 across the 18 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

astro-ph.SR2026

The evolutionary history of ultra-compact accreting binaries. II. HST spectroscopy of two eclipsing AM CVn stars

W. Yu, A. F. Pala, T. Kupfer +50

AM CVn stars are ultra-compact binaries in which a white dwarf (WD) accretes helium-rich material from a hydrogen-deficient donor. They are promising mHz gravitational-wave sources…

astro-ph.SR2026

A systematic survey for hypervelocity runaways from thermonuclear supernovae

Kareem El-Badry, Klaus Werner, Ken J. Shen +16

The explosion of a white dwarf (WD) in a close binary can launch a surviving runaway star at velocities of ≳1000kms−1. Such runaways provide a direct probe of…

astro-ph.SR2026

No Period Change in Two Long-Period AM CVn Binaries

Matthew J. Green, Thomas R. Marsh, Jan van Roestel +25

Ultracompact binary systems, consisting of two compact objects in an orbit ≲0.5R⊙​, should exhibit measurable rates of orbital period change (P˙=0) due t…

astro-ph.SR2026

Thermal Evolution of the Central Star in Pa 30

Anthony L. Piro, Yossef Zenati, Tin Long Sunny Wong

Pa 30 has been identified as the nebular remnant of the historical SN 1181. It is host to a hot (≈200,000K) central star (WD J005311) with a fast wind ($\approx16,0…

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