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| Miscellaneous :
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Malizia et al. 2011:ATel 3290
- Swift follow up
- X-ray spectrum:black body kT~85 eV + power law Γ~2.6
- R~14.7, B~16.2, J~13.9, H~13.6 and K~13.5
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Pavan et al. 2011 A&A:
- Multi instrumental archival data analysis and search for counterparts.
- XMM data => source composed three different emitting regions: a 4-arcmin extended
cometary-like tail (also detected by Swift, ASCA and Einstein) + 2 sources separated by ~22 arcsec
- One of the 2 sources is extended (8.1")
- No detection of IR or Optical counterparts within 90% XMM error circle
- Possible radio counterpart (in MGPS-2 @ ) F843 MHz=24.2 mJy, close to the 8.1" extended source
- All 3 components well fitted with a power-law model
- Spectral and timing analysis => pulsar wind nebula produced by a high-velocity pulsar
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Tomsick et al. 2012 ApJ:
- Chandra observation => complexity of the morphology of the source
- Composed of a point source + extension pointing to the North East direction
(towards SNR MSH 11-61A) and ~4 arcmin long tail, perpendicular to the NE extension
- Spectral analysis of the extended emission is presented, and the overall properties
of the system discussed.
- All results consistent with point source = pulsar (although no pulsations detected in the radio observations)
- IGR source is a likely Pwin then
- The NE extension = result of a bow shock due to pulsar motion through the ISM
- Association with the SNR MSH 11-61A suggested =>would imply a large kick velocity of 2400-2900 km s-1 for the pulsar.
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Pavan et al. 2014 A&A:
- Investigation of the 4' long tail (jet-like- structire invesigated with Chandra and ATCA observations
- The structure is a true plsar's jet
- Highly collimated over 11pc, displays precession-like modulation precession period 66yr, precessing cone 45°
angle to the line of sight ~ 50°
- Spin axis of the NS almost perpendicular to the direction of motion => spin axis perpendicular to the
direction of the kick received at the SN explosions
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