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researcher

L Wang

3 papers here

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

author position
  • first author1
  • middle author1

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

fields
  • astro-ph.SR2
  • astro-ph.HE1
ORCID 0000-0002-9803-166X
same name
  • L Wang — 1 paper
  • L Wang — 1 paper

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
20162019
most citedEvidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0

25 citations · 63 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2019★ 16 cited

Phase-Resolved Spectroscopy of Gaia14aae: Line Emission From Near the White Dwarf Surface

M. J. Green, T. R. Marsh, D. Steeghs +8

AM CVn binaries are a class of ultracompact, hydrogen-deficient binaries, each consisting of a white dwarf accreting helium-dominated material from a degenerate or semi-degenerate…

astro-ph.SR2018★ 25 cited

Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0

A. F. Pala, B. T. Gänsicke, T. R. Marsh +21

We present high-time-resolution photometry and phase-resolved spectroscopy of the short-period (Porb​=80.52min) cataclysmic variable SDSS J123813.73-033933.…

astro-ph.HE2016★ 22 cited

System mass constraints for the accreting millisecond pulsar XTE J1814-338 using Bowen fluorescence

L. Wang, D. Steeghs, J. Casares +5

We present phase-resolved spectroscopy of the millisecond X-ray pulsar XTE J1814-338 obtained during its 2003 outburst. The spectra are dominated by high-excitation emission lines…

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