The long helical jet of the Lighthouse nebula, IGR J11014-6103

@article{Pavan2013TheLH,
  title={The long helical jet of the Lighthouse nebula, IGR J11014-6103},
  author={Lucia Pavan and P. Bordas and Gerd Puehlhofer and Miroslav D. Filipovi{\'c} and Ain Y. De Horta and Andrew O’Brien and Matteo Balbo and Roland Walter and Enrico Bozzo and Carlo Ferrigno and Evan J. Crawford and Luigi Stella},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2013}
}
Jets from rotation-powered pulsars have so far only been observed in systems moving subsonically trough their ambient medium and/or embedded in their progenitor supernova remnant (SNR). Supersonic runaway pulsars are also expected to produce jets, but they have not been confirmed so far. We investigated the nature of the jet-like structure associated to the INTEGRAL source IGR J11014-6103 (the "Lighthouse nebula"). The source is a neutron star escaping its parent SNR MSH 11-61A supersonically… 

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References

SHOWING 1-10 OF 55 REFERENCES

The Variable Jet of the Vela Pulsar

Observations of the Vela pulsar-wind nebula (PWN) with the Chandra X-Ray Observatory have revealed a complex, variable PWN structure, including inner and outer arcs, a jet in the direction of the

The Guitar nebula: a bow shock from a slow-spin, high-velocity neutron star

THE observable interactions of neutron stars with their local environment provide an opportunity for measuring the properties of both relativistic pulsar winds and the surrounding interstellar

The pulsar B2224+65 and its jets: a two epoch X-ray analysis

We present an X-ray morphological and spectroscopic study of the pulsar B2224+65 and its apparent jet-like X-ray features based on two epoch Chandra observations. The main X-ray feature, which shows

IS IGR J11014–6103 A PULSAR WITH THE HIGHEST KNOWN KICK VELOCITY?

We report on Chandra X-ray and Parkes radio observations of IGR J11014–6103, which is a possible pulsar wind nebula with a complex X-ray morphology and a likely radio counterpart. With the superb

PSR J0357+3205: THE TAIL OF THE TURTLE

Using a new XMM-Newton observation, we have characterized the X-ray properties of the middle-aged radio-quiet γ-ray pulsar J0357+3205 (named Morla) and its tail. The X-ray emission from the pulsar is

XMM-NEWTON OBSERVATION OF PSR B2224+65 AND ITS JET

We have investigated the pulsar PSR B2224+65 and its X-ray jet with XMM-Newton. Apart from the long X-ray jet which is almost perpendicular to the direction of proper motion, a putative extended

On the X-ray feature associated with the Guitar nebula

Context. A mysterious X-ray nebula, showing a remarkably linear geometry, was recently discovered close to the Guitar Nebula, the bow-shock nebula associated with B2224+65, which is the fastest

PSR J0357+3205: A FAST-MOVING PULSAR WITH A VERY UNUSUAL X-RAY TRAIL

The middle-aged PSR J0357+3205 is a nearby, radio-quiet, bright γ-ray pulsar discovered by the Fermi mission. Our previous Chandra observation revealed a huge, very peculiar structure of diffuse

IGR J11014-6103: a newly discovered pulsar wind nebula?

Context. IGR J11014-6103 is one of the still unidentified hard X-ray INTEGRAL sources, reported for the first time in the 4th IBIS/ISGRI catalog. Aims. We investigated the nature of IGR J11014-6103

On the origin of the jet-like radio/X-ray morphology of G290.1–0.8

Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well understood. Several remnants present distorted radio or X-ray shells with jet-like structures.
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