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Ying-Han Mao

4 papers hereh-index 28 citations8 works total

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author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

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  • astro-ph.HE4
same name
  • Ying-Han Mao — 2 papers

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

most citedFormation of millisecond pulsar-helium star binaries

4 citations · 4 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

How Beaming Shapes the Demographics of Ultraluminous X-ray Sources?

Ying-Han Mao, Xiang-Dong Li

Ultraluminous X-ray sources (ULXs) are off-nuclear compact objects with apparent luminosities above 10^39 erg/s, often exceeding the Eddington limit for stellar-mass black holes. B…

astro-ph.HE2025★ 4 cited

Formation of millisecond pulsar-helium star binaries

Zhu-Ling Deng, Xiang-Dong Li, Yong Shao +2

PSR J1928+1815, the first recycled pulsar-helium (He) star binary discovered by the Five-hundred-meter Aperture Spherical radio Telescope, consists of a 10.55 ms pulsar and a compa…

astro-ph.HE2025

A statistical study of type II outbursts of XRPs: Brighter accreting pulsars rotate faster

Shan-Shan Weng, Xiao-Tian Xu, Han-Long Peng +6

X-ray pulsars (XRPs) consist of a magnetized neutron star (NS) and an optical donor star. The NS accretes matter from the donor star producing pulsed X-ray emission. In most cases…

astro-ph.HE2025

A binary origin of ultra-long period radio pulsars

Ying-Han Mao, Xiang-Dong Li, Dong Lai +2

We propose a possible binary evolution model for the formation of ultra-long period pulsars (ULPPs). The model involves two key stages: first, a neutron star (NS) in wide binaries…

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