Kinematics of the Pencil nebula (RCW 37) and its association with the young Vela supernova remnant RX J0852.0-4622

The association between the Pencil nebula (RCW 37, NGC 2736), the Vela X-ray fragment D/Dand the recently discovered new X-ray supernova remnant (RX J0852.0−4622) in Vela is investigated. Recently published Chandra images of D/Dare compared with optical images of RCW 37 and confirm the close association of the two objects. New optical line profiles of RCW 37 from an extended slit position passing through this unusual optical nebula are presented. They reveal a partial velocity ellipse with expansion velocities of around 120 km s −1 . Various scenarios for the origin of the nebula are considered and the evidence of a link with RX J0852.0−4622 is reviewed. A funnel of gas similar to those in the Crab and DEM34a supernova remnants (SNRs) is not ruled out but a more plausible explanation may be that a 'wavy sheet' is responsible. We suggest that RX J0852.0−4622 is located within the older larger Vela SNR and that some of the X-ray gas from RX J0852.0−4622 has collided with the dense H I wall of the older remnant. This gives rise to the morphology and velocity structure of the optical emission and explains the unusual X-ray emission from this portion of the supernova remnant. If our hypothesis is correct, a distance prediction of 250 ± 30 pc can be made, based on recent measurements of the distance to the old Vela SNR. This is at the lower end of the range of distances quoted in the literature and would confirm the unusual nature of this young nearby supernova remnant.