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Shuai-Bing Ma

4 papers here

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph.HE4

identity via Semantic Scholar / OpenAlex

activity
20172021
most citedBright "Merger-nova" Emission Powered by Magnetic wind from a New-Born Black Hole

30 citations · 42 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2021★ 12 cited

Constraining Properties of GRB Central Engines with X-ray flares

Shuang-Xi Yi, Wei Xie, Shuai-Bing Ma +2

X-ray flares in gamma-ray bursts (GRBs) are believed to be generated by the late activities of central engine, and thus provide an useful tool to diagnose the properties of central…

astro-ph.HE2021

Detectability of "Merger-nova" emission from a long-lived magnetar in short gamma-ray bursts

Yong Yuan, Hou-Jun Lü, Hao-Yu Yuan +3

One possible progenitor of short gamma-ray bursts (GRBs) is thought to be from a double neutron star (NS) merger, and the remnant of such a merger may be a supramassive NS, which i…

astro-ph.HE2019

G4.8+6.2, a possible kilonova remnant?

Yu Liu, Yuan-Chuan Zou, Bing Jiang +3

Kilonova explosions typically release ∼1050−51 erg in kinetic energy, which is sufficient to constitute a kilonova remnant (KNR); however, it has not yet been confirmed. I…

astro-ph.HE2017★ 30 cited

Bright "Merger-nova" Emission Powered by Magnetic wind from a New-Born Black Hole

Shuai-Bing Ma, Wei-Hua Lei, He Gao +4

Mergers of neutron star-neutron star (NS-NS) or neutron star-black hole (NS-BH) binaries are candidate sources of gravitational waves (GWs). At least a fraction of the merger remna…

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