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researcher

Tom Oosterloo

5 papers here

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

author position
  • middle author5

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • astro-ph1
  • astro-ph.SR1
ORCID 0000-0002-0616-6971

identity via Semantic Scholar / OpenAlex

activity
20022011
most citedA collisional origin for the Leo ring

55 citations · 72 across the 5 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.SR2010★ 15 cited

Radio observations of candidate magnetic O stars

R. S. Schnerr, K. L. J. Rygl, A. J. van der Horst +5

Context: Some O stars are suspected to have to have (weak) magnetic fields because of the observed cyclical variability in their UV wind-lines. However, direct detections of these…

astro-ph.CO2010★ 55 cited

A collisional origin for the Leo ring

Leo Michel-Dansac, Pierre-Alain Duc, Frederic Bournaud +6

Extended HI structures around galaxies are of prime importance to probe galaxy formation scenarios. The giant HI ring in the Leo group is one of the largest and most intriguing HI…

astro-ph.CO2010

Detection of the H92alpha recombination line from NGC 4945

A. L. Roy, T. Oosterloo, W. M. Goss +1

Context. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio recombination lines (RRLs), whose strength can be used as a diagnostic of the ionization ra…

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