High-energy emission from the composite supernova remnant MSH 15-56

Tea Temim, Patrick Slane, Daniel Castro, Paul P. Plucinsky, Joseph (Yosi) Gelfand, John R. Dickel

Research output: Contribution to journalArticle

Abstract

MSH 15-56 (G326.3-1.8) is a composite supernova remnant (SNR) that consists of an SNR shell and a displaced pulsar wind nebula (PWN) in the radio. We present XMM-Newton and Chandra X-ray observations of the remnant that reveal a compact source at the tip of the radio PWN and complex structures that provide evidence for mixing of the supernova (SN) ejecta with PWN material following a reverse shock interaction. The X-ray spectra are well fitted by a non-thermal power-law model whose photon index steepens with distance from the presumed pulsar, and a thermal component with an average temperature of 0.55 keV. The enhanced abundances of silicon and sulfur in some regions, and the similar temperature and ionization timescale, suggest that much of the X-ray emission can be attributed to SN ejecta that have either been heated by the reverse shock or swept up by the PWN. We find one region with a lower temperature of 0.3 keV that appears to be in ionization equilibrium. Assuming the Sedov model, we derive a number of SNR properties, including an age of 16,500 yr. Modeling of the γ-ray emission detected by Fermi shows that the emission may originate from the reverse shock-crushed PWN.

Original languageEnglish (US)
Article number61
JournalAstrophysical Journal
Volume768
Issue number1
DOIs
StatePublished - May 1 2013

Fingerprint

supernova remnants
pulsars
nebulae
composite materials
energy
ejecta
shock
ionization
supernovae
radio
x rays
silicon
XMM-Newton telescope
power law
newton
temperature
sulfur
shell
rays
timescale

Keywords

  • gamma rays: ISM
  • ISM: individual objects (MSH 1556, G326.1?1.8)
  • ISM: supernova remnants
  • pulsars: general
  • X-rays: ISM

ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

High-energy emission from the composite supernova remnant MSH 15-56. / Temim, Tea; Slane, Patrick; Castro, Daniel; Plucinsky, Paul P.; Gelfand, Joseph (Yosi); Dickel, John R.

In: Astrophysical Journal, Vol. 768, No. 1, 61, 01.05.2013.

Research output: Contribution to journalArticle

Temim, Tea ; Slane, Patrick ; Castro, Daniel ; Plucinsky, Paul P. ; Gelfand, Joseph (Yosi) ; Dickel, John R. / High-energy emission from the composite supernova remnant MSH 15-56. In: Astrophysical Journal. 2013 ; Vol. 768, No. 1.
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