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researcher

O. Cohen

23 papers hereh-index 15726 citations24 works total

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

author position
  • first author11
  • middle author6
  • last author3

Across the 20 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR19
  • astro-ph.EP4
same name
  • O. Cohen — 66 papers, h 30
  • O. Cohen — 32 papers, h 47
  • O. Cohen — 9 papers, h 11
  • O. Cohen — 8 papers, h 7
  • O. Cohen — 8 papers, h 7
  • O. Cohen — 5 papers, h 2

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
20092026
most citedThe Revolution Revolution: magnetic morphology driven spin-down

136 citations · 1.1k across the 23 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.SR2010★ 76 cited

The Impact of Hot Jupiters on the Spin-down of their Host Stars

O. Cohen, J. J Drake, V. L. Kashyap +2

We present a numerical Magnetohydrodynamic (MHD) study of the dependence of stellar mass and angular momentum- loss rates on the orbital distance to close-in giant planets. We find…

astro-ph.SR2010★ 89 cited

XMM-Newton observations of HD189733 during planetary transits

I. Pillitteri, S. J. Wolk, O. Cohen +4

We report on two XMM-Newton observations of the planetary host star HD189733. The system has a close in planet and it can potentially affect the coronal structure via interactions…

astro-ph.SR2010★ 43 cited

The Coronal Structure of AB Doradus

O. Cohen, J. J. Drake, V. L. Kashyap +2

We perform a numerical simulation of the corona of the young, rapidly rotating K0 dwarf AB Doradus using a global MHD model. The model is driven by a surface map of the radial magn…

astro-ph.SR2010★ 12 cited

Magnetic Structure of Rapidly Rotating FK Comae-Type Coronae

O. Cohen, J. J. Drake, V. L. Kashyap +3

We present a three-dimensional simulation of the corona of an FK Com-type rapidly rotating G giant using a magnetohydrodynamic model that was originally developed for the solar cor…

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