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R. Owen

6 papers hereh-index 7145 citations10 works total

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

author position
  • first author3
  • middle author1
  • last author1

Across the 5 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE2
  • astro-ph1
same name
  • R. Owen — 57 papers, h 32
  • R. Owen — 29 papers, h 28
  • R. Owen — 3 papers, h 38
  • R. Owen — 3 papers
  • R. Owen — 2 papers, h 32
  • R. Owen — 1 paper, h 1

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
20072011
most citedX-ray emission from the extended disks of spiral galaxies

72 citations · 184 across the 6 of their papers we have counts for

collaborators
Showing 2011Show all

3 papers · 1 filter

astro-ph.HE2011★ 38 cited

A new super-soft X-ray source in the Small Magellanic Cloud: Discovery of the first Be/white dwarf system in the SMC?

R. Sturm, F. Haberl, W. Pietsch +5

The Small Magellanic Cloud (SMC) hosts a large number of Be/X-ray binaries, however no Be/white dwarf system is known so far, although population synthesis calculations predict tha…

astro-ph.GA2011★ 17 cited

Constraints on sterile neutrino dark matter from XMM--Newton observation of M33

Enrico Borriello, Maurizio Paolillo, Gennaro Miele +2

Using archival XMM-Newton observations of the diffuse and unresolved components emission in the inner disc of M33 we exclude the possible contribution from narrow line emission in…

astro-ph.HE2011★ 37 cited

IKT 16: A Composite SNR in the SMC

R. A. Owen, M. D. Filipovic, J. Ballet +11

Aims: IKT 16 is an X-ray and radio-faint supernova remnant (SNR) in the Small Magellanic Cloud (SMC). A previous X-ray study of this SNR found a hard X-ray source near its centre.…

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