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researcher

F. Liu

22 papers hereh-index 13 citations5 works total

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

author position
  • sole author1
  • first author6
  • middle author8
  • last author6

Across the 21 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE10
  • astro-ph.GA6
  • astro-ph3
  • astro-ph.CO3
same name
  • F. Liu — 568 papers, h 86
  • F. Liu — 210 papers, h 19
  • F. Liu — 130 papers, h 16
  • F. Liu — 85 papers, h 2
  • F. Liu — 78 papers, h 29
  • F. Liu — 65 papers, h 5

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
19952026
most citedEnhanced tidal disruption rates from massive black hole binaries

144 citations · 913 across the 22 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.HE2023★ 35 cited

Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios

S. Komossa, D. Grupe, A. Kraus +9

The project MOMO (Multiwavelength Observations and Modelling of OJ 287) was set up to test predictions of binary supermassive black hole (SMBH) scenarios and to understand disk-jet…

astro-ph.HE2023★ 26 cited

MOMO VI: Multifrequency radio variability of the blazar OJ 287 from 2015-2022, absence of predicted 2021 precursor-flare activity, and a new binary interpretation of the 2016/2017 outburst

S. Komossa, A. Kraus, D. Grupe +12

Based on our dedicated Swift monitoring program, MOMO, OJ 287 is one of the best-monitored blazars in the X-ray--UV--optical regime. Here, we report results from our accompanying,…

astro-ph.HE2023★ 3 cited

Tracing the Evolution of SMBHs and Stellar Objects in Galaxy Mergers: An Multi-mass Direct N-body Model

Shuo Li, Shiyan Zhong, Peter Berczik +3

By using direct N-body numerical simulations, we model the dynamical co-evolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to…

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