activity
19932025
most citedBlack Hole Growth in Dark Matter and the M_{bh} - σRelation

46 citations · 247 across the 17 of their papers we have counts for

collaborators

17 papers

physics.flu-dyn2025

A Lie Scale Invariance in Fluids with Applications

Richard Henriksen

Lie scale invariance is used to reduce the incompressible Navier-Stokes equations to non-linear ordinary equations. This yields a formulation in terms of logarithmic spirals as ind…

gr-qc2024

An Event Horizon 'Firewall' Undergoing Cosmological Expansion

R N Henriksen, A G Emslie

We embed an object with a singular horizon structure, reminiscent of (but fundamentally different from, except in a limiting case) a black-hole event horizon, in an expanding, sphe…

astro-ph.GA2020★ 12 cited

Helicity in the Large-Scale Galactic Magnetic Field

J. L. West, R. N. Henriksen, K. Ferrière +4

We search for observational signatures of magnetic helicity in data from all-sky radio polarization surveys of the Milky Way Galaxy. Such a detection would help confirm the dynamo…

astro-ph.GA2019★ 20 cited

Evolving Galactic Dynamos and Fits to the Reversing Rotation Measures in the Halo of NGC 4631

Alex Woodfinden, Richard Henriksen, Judith Irwin +1

Rotation measure (RM) synthesis maps of NGC 4631 show remarkable sign reversals with distance from the minor axis in the northern halo of the galaxy on kpc scales. To explain this…

astro-ph.GA2019

A `Numbers' Approach to Astronomical Correlations I: Introduction and Application to galaxy Scaling Relations

R. N. Henriksen, J. A. Irwin

We propose a new systematic method of studying correlations between parameters that describe an astronomical (or any) physical system. We recall that behind Dimensionless scaling l…

astro-ph.GA2018★ 11 cited

CHANG-ES XI: Circular Polarization in the Cores of Nearby Galaxies

Judith A Irwin, Richard N. Henriksen, Marek Wezgowiec +18

We detect 5 galaxies in the CHANG-ES (Continuum Halos in Nearby Galaxies -- an EVLA Survey) sample that show circular polarization (CP) at L-band in our high resolution data sets.…