Thermal and Nonthermal X-Ray Emission in SNR RCW 86

TL;DR

This study analyzes X-ray spectra of supernova remnant RCW 86, revealing the coexistence of thermal and nonthermal emissions, with evidence supporting X-ray synchrotron radiation linked to radio brightness.

Contribution

It provides a detailed spectral analysis combining thermal and nonthermal models, demonstrating the presence of X-ray synchrotron emission in RCW 86.

Findings

Nonthermal X-ray continuum correlates with radio brightness.

Shock velocity estimated at 800 km/s.

Spectral break at 2-4x10^16 Hz indicating synchrotron emission.

Abstract

Supernova remnants may exhibit both thermal and nonthermal X-ray emission. Such remnants can be distinguished by the weakness of their X-ray lines, because of the presence of a strong nonthermal X-ray continuum. RCW 86 is a remnant with weak lines, resulting in low and peculiar abundances when thermal models alone are used to interpret its X-ray spectrum. This indicates the presence of a strong nonthermal synchrotron continuum. We analyze ASCA X-ray spectra of RCW 86 with the help of both nonequilibrium ionization thermal models and nonthermal synchrotron models. A two-temperature thermal model and a simple nonthermal model with an exponential cutoff (plus interstellar absorption) give reasonable results. We obtain blast wave velocity of 800 km/s, the shock ionization age of 1-3x10^11 s/cm^3, and the break in nonthermal spectra at 2-4x10^16 Hz. The strength of nonthermal continuum correlates well with the radio brightness in the bright SW section of the remnant. This is convincing evidence for X-ray synchrotron emission in RCW 86.