Articulo
A likely optical counterpart of the G292.0+1.8 pulsar wind nebula
Fecha
2008Registro en:
15010003
WOS:000261697900022
no scielo
eid=2-s2.0-57649228002
Institución
Resumen
Context. G292.0+1.8 is a Cas A-like supernova remnant containing the young pulsar PSR J1124-5916, which powers a compact torus-like pulsar wind nebula with a jet visible in X-rays. Aims. We have performed deep optical observations of the pulsar field to d