Proper Motions of H-alpha filaments in the Supernova Remnant RCW 86

TL;DR

This study measures the proper motions of H-alpha filaments in RCW 86, revealing shock velocities and their variation, and compares optical and X-ray data to infer shock properties and remnant distance.

Contribution

First proper motion measurements of H-alpha filaments in RCW 86 using VLT data, providing insights into shock velocities and their implications for remnant properties.

Findings

Proper motions of 0.10 +/- 0.02 arcsec/yr corresponding to ~1200 km/s.

Shock velocities range from below 700 km/s to above 2200 km/s.

Optical proper motions are lower than X-ray measurements, consistent with proton temperature data.

Abstract

We present a proper motion study of the eastern shock-region of the supernova remnant RCW 86 (MSH 14-63, G315.4-2.3), based on optical observations carried out with VLT/FORS2 in 2007 and 2010. For both the northeastern and southeastern regions, we measure an average proper motion of H-alpha filaments of 0.10 +/- 0.02 arcsec/yr, corresponding to 1200 +/- 200 km/s at 2.5kpc. There is substantial variation in the derived proper motions, indicating shock velocities ranging from just below 700 km/s to above 2200 km/s. The optical proper motion is lower than the previously measured X-ray proper motion of northeastern region. The new measurements are consistent with the previously measured proton temperature of 2.3 +/- 0.3 keV, assuming no cosmic-ray acceleration. However, within the uncertainties, moderately efficient (< 27 per cent) shock acceleration is still possible. The combination of optical proper motion and proton temperature rule out the possibility that RCW 86 has a distance less than 1.5kpc. The similarity of the proper motions in the northeast and southeast is peculiar, given the different densities and X-ray emission properties of the regions. The northeastern region has lower densities and the X-ray emission is synchrotron dominated, suggesting that the shock velocities should be higher than in the southeastern, thermal X-ray dominated, region. A possible solution is that the H-alpha emitting filaments are biased toward denser regions, with lower shock velocities. Alternatively, in the northeast the shock velocity may have decreased rapidly during the past 200yr, and the X-ray synchrotron emission is an afterglow from a period when the shock velocity was higher.