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Xiaotian Xu

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.SR2
  • astro-ph.HE1
ORCID 0000-0001-9565-9462
same name
  • Xiaotian Xu — 5 papers
  • Xiaotian Xu — 2 papers
  • Xiaotian Xu — 1 paper
  • Xiaotian Xu — 1 paper
  • Xiaotian Xu — 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
20212023
most citedDetailed models of interacting short-period massive binary stars

88 citations · 110 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2023★ 7 cited

Back to the Starting Point: on the Simulation of Initial Magnetic Fields and Spin Periods of Non-accretion Pulsars

Kun Xu, Hao-Ran Yang, Ying-Han Mao +3

Neutron stars (NSs) play essential roles in modern astrophysics. Magnetic fields and spin periods of newborn (zero age) NSs have large impact on the further evolution of NSs, which…

astro-ph.SR2022★ 15 cited

The spins of stripped B stars support magnetic internal angular momentum transport

C. Schürmann, N. Langer, X. Xu +1

In order to predict the spins of stellar remnants we need to understand the evolution of the internal rotation of stars, and to identify at which stage the rotation of the contract…

astro-ph.SR2021★ 88 cited

Detailed models of interacting short-period massive binary stars

K. Sen, N. Langer, P. Marchant +10

About a quarter of massive binary stars undergo mass transfer while both stars burn hydrogen at their cores, first on the thermal and then on the nuclear timescale. The nuclear tim…

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