A multiwavelength study of the supernova remnant G296.8-0.3

TL;DR

This study combines X-ray, radio, and infrared observations to analyze the structure, physical properties, and possible evolutionary scenarios of the supernova remnant G296.8-0.3, revealing its thermal X-ray emission, peculiar morphology, and a potential central compact object.

Contribution

It provides the first detailed multiwavelength analysis of G296.8-0.3, identifying its thermal X-ray emission, complex morphology, and a candidate central compact object, advancing understanding of its physical state and evolution.

Findings

X-ray emission correlates with radio morphology

Remnant is likely distant (>9 kpc) with thermal X-ray spectrum

Detected point source consistent with a central compact object

Abstract

We report XMM-Newton observations of the Galactic supernova remnant G296.8-0.3, together with complementary radio and infrared data. The spatial and spectral properties of the X-ray emission, detected towards G296.8-0.3, was investigated in order to explore the possible evolutionary scenarios and the physical connexion with its unusual morphology detected at radio frequencies. G296.8-0.3 displays diffuse X-ray emission correlated with the peculiar radio morphology detected in the interior of the remnant and with the shell-like radio structure observed to the northwest side of the object. The X-ray emission peaks in the soft/medium energy range (0.5-3.0 keV). The X-ray spectral analysis confirms that the column density is high (NH \sim 0.64 x 10^{22} cm^{-2}) which supports a distant location (d>9 kpc) for the SNR. Its X-ray spectrum can be well represented by a thermal (PSHOCK) model, with kT \sim 0.86 keV, an ionization timescale of 6.1 x 10^{10} cm^{-3} s, and low abundance (0.12 Z_sun). The 24 microns observations show shell-like emission correlated with part of the northwest and southeast boundaries of the SNR. In addition a point-like X-ray source is also detected close to the geometrical center of the radio SNR. The object presents some characteristics of the so-called compact central objects (CCO). Its X-ray spectrum is consistent with those found at other CCOs and the value of NH is consistent with that of G296.8-0.3, which suggests a physical connexion with the SNR.