The Physics of Supernova Remnant Blast Waves. II. Electron-Ion Equilibration in DEM L71 in the Large Magellanic Cloud

We present analysis and modeling of X-ray spectra from the blast wave shock of DEM L71 in the Large Magellanic Cloud. This remnant exhibits widespread Balmer-dominated emission characteristic of nonradiative shocks in partially neutral gas. We have used both Chandra ACISS data and optical Fabry-Perot spectra of the blast wave to measure the electron and proton temperatures, respectively. In principle, when combined, these measurements can determine the degree of electron-ion temperature equilibration (g0 ≡ Te/Tp) immediately behind the shock front. In our X-ray analysis we fit Chandra spectra of three nested regions behind the blast wave under three different scenarios: (1) a planar, initially unequilibrated shock (g0 = me/mp ), where the downstream electron and proton temperatures equilibrate through Coulomb collisions, (2) a planar, immediately equilibrated shock (g0 = 1) and (3) a spherical, equilibrated shock under Sedov evolution. Using independent measurements of Te and Tp we find that the X-ray spectra from the fastest blast wave locations (Vs ∼ 700− 1000 km s−1 ) are consistent with little or no equilibration at the shock front and are inconsistent with full equilibration. In contrast, spectra from regions showing slower blast wave speeds (Vs ∼ 400−600 km s−1 ) allow full equilibration but exclude zero equilibration. In order to directly constrain the initial equilibration, we incorporated our knowledge of the proton temperatures into our X-ray models to build planar shock models that allowed for a variable g0. This model confirmed and strengthened the above results. Specifically, we found that X-ray spectra from an intermediate velocity shock (Vs ∼ 800 km s−1 ) were consistent with intermediate equilibration, excluding both g0 = me/mp and g0 = 1 at greater than 1σ. Overall, our results support the picture of decreasing electron-ion equilibration with increasing shock speed found from previous studies of optical spectra in other Balmer-dominated supernova remnants. Subject headings: ISM: individual (DEM L71, 0505−67.9) – shock waves – supernova remnants – X-rays: