Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels

Abstract

We present the results of the combined analysis of three XMM-Newton EPIC observations of the northern rim of the Vela SNR. The three pointings cover an area of ~10 pc^2 (at 250 pc) behind the main shock front and we aim at studying with high resolution the spatial distribution of the physical and chemical properties of the X-ray emitting plasma on this large scale. We produce count-rate images and equivalent width maps of the Ne IX and Mg XI emission blends. We also perform a spatially resolved spectral analysis of a set of physically homogeneous regions. We reveal physical and chemical inhomogeneities in the X-ray emitting plasma. In particular, we find large variations of the O, Ne, Mg, and Fe abundances. In some bright knots we also find unexpectedly enhanced Ne and Mg abundances, with values significantly larger than solar. Our results support a possible association of a few X-ray emitting knots with previously undetected residuals of stellar fragments (i. e. shrapnels) observed, in projection, inside the Vela shell.

Accepted for publication in The Astrophysical Journal. For the version of the paper with high resolution images, please see http://www.astropa.unipa.it/Library/preprint.html

References in corpus (3)

• The X-ray emission of the supernova remnant W49B observed with XMM-Newton
• Spatially Resolved X-ray Spectroscopy of Vela Shrapnel A
• Shock-cloud interaction in the Vela SNR II. Hydrodynamic model

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