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researcher

A. Wagner

37 papers hereh-index 201.5k citations53 works total

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

author position
  • first author5
  • middle author22
  • last author10

Across the 37 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA25
  • astro-ph.HE6
  • astro-ph.CO4
  • astro-ph1
  • astro-ph.IM1
same name
  • A. Wagner — 120 papers, h 32
  • A. Wagner — 40 papers, h 22
  • A. Wagner — 29 papers, h 39
  • A. Wagner — 24 papers
  • A. Wagner — 24 papers, h 7
  • A. Wagner — 22 papers, h 25

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
20082023
most citedDriving Outflows with Relativistic Jets and the Dependence of AGN Feedback Efficiency on ISM Inhomogeneity

300 citations · 2.4k across the 37 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.CO2019★ 40 cited

Cusp-to-core transition in low-mass dwarf galaxies induced by dynamical heating of cold dark matter by primordial black holes

Pierre Boldrini, Yohei Miki, Alexander Y. Wagner +3

We performed a series of high-resolution N-body simulations to examine whether dark matter candidates in the form of primordial black holes (PBHs) can solve the cusp-core problem…

astro-ph.GA2019★ 16 cited

Searching for signs of jet-driven negative feedback in the nearby radio galaxy UGC 05771

Henry R. M. Zovaro, Nicole P. H. Nesvadba, Robert Sharp +4

Hydrodynamical simulations predict that the jets of young radio sources can inhibit star formation in their host galaxies by injecting heat and turbulence into the interstellar med…

astro-ph.GA2019★ 31 cited

Feedback from low-luminosity radio galaxies: B2 0258+35

Suma Murthy, Raffaella Morganti, Tom Oosterloo +6

Low-luminosity radio-loud active galactic nuclei (AGN) are of importance in studies concerning feedback from radio AGN since a dominant fraction of AGN belong to this class. We rep…

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