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The 'Rabbit': A Potential Radio Counterpart of GeV J1417−6100
- Source :
- The Astrophysical Journal. 515:712-720
- Publication Year :
- 1999
- Publisher :
- American Astronomical Society, 1999.
-
Abstract
- We have mapped the radio emission in the error ellipse of GeV J1417-6100 (2EGS J1418-6049) at 13cm and 20cm using the Australia Telescope Compact Array. We find a large shell with extended wings, at the edge of which is a non-thermal, polarized structure with a center filled morphology (the `Rabbit'), coincident with an extended, hard X-ray source. We discuss the various sources seen within the ellipse as potential counterparts of the gamma-ray source. We conclude that the most likely scenario is that the Rabbit is a wind nebula surrounding a radio-quiet gamma-ray pulsar.<br />14 pages, 6 figures, to be published in the Astrophysical Journal
- Subjects :
- Physics
Nebula
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics (astro-ph)
Shell (structure)
FOS: Physical sciences
Astronomy and Astrophysics
Astrophysics
Ellipse
law.invention
Telescope
Pulsar
Space and Planetary Science
law
Coincident
Astrophysics::Solar and Stellar Astrophysics
Rabbit (cipher)
Subjects
Details
- ISSN :
- 15384357 and 0004637X
- Volume :
- 515
- Database :
- OpenAIRE
- Journal :
- The Astrophysical Journal
- Accession number :
- edsair.doi.dedup.....bad2937d9aed7b426d887e49bfd66538
- Full Text :
- https://doi.org/10.1086/307058