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Bo Ma

4 papers here

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

author position
  • middle author2
  • last author2

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

fields
  • astro-ph.SR4
same name
  • Bo Ma — 8 papers
  • Bo Ma — 7 papers
  • Bo Ma — 6 papers, h 2
  • Bo Ma — 6 papers, h 1
  • Bo Ma — 4 papers, h 5
  • Bo Ma — 4 papers, h 3

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

collaborators

4 papers

astro-ph.SR2026

Searching for White Dwarf Candidates Formed Through Binary evolution in Star Clusters

Huahui Yan, Li Wang, David R. Miller +11

White dwarfs (WDs), the evolutionary endpoints of most stars, can form through both single-star and binary channels. While single-star evolutionary models enable reliable WD age es…

astro-ph.SR2026

Fates of the sub-stellar objects (FOSSO) I. Fates of the known brown dwarfs in main-sequence--BD binaries

Zhangliang Chen, Hongming Jin, Hongwei Ge +4

Context. Understanding the survival and orbital evolution of brown dwarf (BD) companions during the post-main-sequence (MS) evolution of their host stars is increasingly important,…

astro-ph.SR2025

A magnetic white dwarf formed through a binary merger within 35 million years

Huahui Yan, Jiamao Lin, Rizhong Zheng +15

White dwarfs (WDs) represent the final evolutionary stage of most stars, typically originating from progenitor stars with masses below approximately 8 M⊙​ to 10 M⊙​…

astro-ph.SR2025

Discovery and characterization of ZTF J0112+5827: An 80.9-minute polar with strong cyclotron features

Jiamao Lin, Liangliang Ren, Chengyuan Li +9

We report the discovery and characterization of ZTF J0112+5827, a new magnetic cataclysmic variable with an orbital period of 80.9 minutes. ROSAT observations revealed X-ray emissi…

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