Optical Observations of PSR J0205+6449
arXiv:0807.0983 · doi:10.1111/j.1365-2966.2008.13693.x
Abstract
PSR J0205+6449 is a X-ray and radio pulsar in supernova remnant 3C 58. We report on observations of the central region of 3C 58 using the 4.2-m William Herschel Telescope with the intention of identifying the optical counterpart of PSR J0205+6449 and characterising its pulsar wind nebula. Around the pulsar position we identified extended emission with a magnitude of $B = 23 \fm 97 \pm 0.10$, $V = 22 \fm 95 \pm 0.05$ and $R = 22 \fm 15 \pm 0.03$ consistent with a pulsar wind nebula. From the R-band image we identified three knots with = $24 \fm 08 \pm 0.07$ (o1), $24 \fm 15 \pm 0.07$ (o2) and $24 \fm 24 \pm 0.08$ (o3). We confirm the presence of an optical pulsar wind nebula around PSR J0205+6449 and give an upper limit of 24 for the optical magnitude of the pulsar. Furthermore we make the tentative suggestion that our object o1, with an 24.08 is the optical counterpart. If confirmed the pulsar would have an and an optical efficiency of about 5% of the Crab pulsar. Such a low efficiency is more consistent with the characteristic age of the pulsar rather than that of SN 1181.
The paper contains 3 figures and 3 tables, accepted for publication in MNRAS
References in corpus (7)
- Discovery of X-ray Pulsations from the Compact Central Source in the Supernova Remnant 3C 58
- Discovery of radio pulsations from the X-ray pulsar J0205+6449 in supernova remnant 3C58 with the Green Bank Telescope
- Radio Images of 3C 58: Expansion and Motion of its Wisp
- A Shell of Thermal X-ray Emission Associated with the Young Crab-like Remnant 3C58
- Optical identification of the 3C 58 pulsar wind nebula
- Implications of the Optical Observations of Neutron Stars
- OPTIMA: A Photon Counting High-Speed Photometer
Cited by in corpus (7)
- A Thorough Investigation of Distance and Age of the Pulsar Wind Nebula 3C58
- Core collapse supernova remnants with ears
- The Proper Motion of PSR J0205+6449 in 3C 58
- The PSR J1124-5916 wind nebula in the near-infrared
- A likely optical counterpart of the G292.0+1.8 pulsar wind nebula
- Optical Observations of PSR J0205+6449 - the next optical pulsar?
- A polarized view of the young Pulsar Wind Nebula 3C 58 with IXPE