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Cited by 270

The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.

Gamma-ray binaries: pulsars in disguise?

Open access
Dubus, G.·2006·Astronomy & Astrophysics
DOI 10.1051/0004-6361:20054779
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Abstract

Context.LS 5039 and LS I+61°303 are unique amongst high-mass X-ray binaries (HMXB) for their spatially-resolved radio emission and their counterpart at >GeV gamma-ray energies, canonically attributed to non-thermal particles in an accretion-powered relativistic jet. The only other HMXB known to emit very high-energy (VHE) gamma-rays, PSR B1259-63, harbours a non-accreting millisecond pulsar.

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Crossref · 10.1051/0004-6361:20054779

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Metadata

Authors
Dubus, G.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2006-09
Volume
456
Issue
3
Pages
801-817
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361:20054779
OpenAlex
W2016271096
Cited by
270
References
14
FWCI
16.12
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Gamma-ray binaries: pulsars in disguise? https://app.cochat.ai/papers/10.1051/0004-6361:20054779
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Dubus, G. (2006). Gamma-ray binaries: pulsars in disguise? Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20054779

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.