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L. M. Song

4 papers hereh-index 347 citations4 works total

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

author position
  • last author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.HE1
same name
  • L. M. Song — 11 papers, h 9
  • L. M. Song — 5 papers, h 4
  • L. M. Song — 3 papers, h 4
  • L. M. Song — 3 papers, h 3
  • L. M. Song — 2 papers, h 1
  • L. M. Song — 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
20032018
most citedPair loading in Gamma-Ray Burst Fireball And Prompt Emission From Pair-Rich Reverse Shock

22 citations · 56 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2018★ 16 cited

Time evolution of the X-ray and gamma-ray fluxes of the Crab pulsar

L. L. Yan, M. Y. Ge, F. J. Lu +5

We studied the evolution of the X-ray and gamma-ray spectra of the Crab pulsar utilizing the 11-year observations from the Rossi X-ray Timing Explorer (RXTE) and 9-year observation…

astro-ph2004★ 18 cited

Prompt Ultraviolet-to-Soft-X-Ray Emission of Gamma-Ray Bursts: Application to GRB 031203?

Zhuo Li, Li-Ming Song

We discuss the prompt emission of GRBs, allowing for γγ pair production and synchrotron self-absorption. The observed hard spectra suggest heavy pair-loading in GRBs. The re-emis…

astro-ph2003

X-ray afterglows of gamma-ray bursts in the synchrotron self-Compton dominated regime

Zhuo Li, L. M. Song

We consider in this paper the effect of synchrotron self-Compton process on X-ray afterglows of gamma-ray bursts. We find that for a wide range of parameter values, especially for…

astro-ph2003★ 22 cited

Pair loading in Gamma-Ray Burst Fireball And Prompt Emission From Pair-Rich Reverse Shock

Zhuo Li, Z. G. Dai, T. Lu +1

Gamma-ray bursts (GRBs) are believed to originate from ultra-relativistic winds/fireballs to avoid the "compactness problem". However, the most energetic photons in GRBs may still…

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