The G292.0+1.8 pulsar wind nebula in the mid-infrared

Context. G292.0+1.8 is a Cas A-like supernova remnant that contains the young pulsar PSR J1124-5916 powering a compact torus-like pulsar wind nebula visible in X-rays. A likely counterpart to the nebula has been detected in the optical VRI bands. Aims. To confirm the counterpart candidate nature, we...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2009-12, Vol.508 (2), p.855-858
Hauptverfasser:	Zyuzin, D. A., Danilenko, A. A., Zharikov, S. V., Shibanov, Yu. A.
Format:	Artikel
Sprache:	eng
Schlagworte:	infrared: general ISM: individual objects: G292.0+1.8 ISM: supernova remnants outflows pulsars: individual: PSR J1124-5916 radiation mechanisms: non-thermal stars: winds
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