SIMBAD references

2009MNRAS.395..351T - Mon. Not. R. Astron. Soc., 395, 351-357 (2009/May-1)

Numerical model for the SNR DEM L316: simulated X-ray emission.

TOLEDO-ROY J.C., VELAZQUEZ P.F., DE COLLE F., GONZALEZ R.F., REYNOSO E.M., KURTZ S.E. and REYES-ITURBIDE J.

Abstract (from CDS):

We present a two-component supernova remnant model for the case of Magellanic remnant DEM L316 obtained from two-dimensional, axisymmetric hydrodynamic simulations. We study different scenarios which consider a possible collision between the shells and also the effects of thermal conduction. Synthetic X-ray maps were obtained from numerical results in order to directly compare with the observed morphology of this object. We find a good agreement is achieved when thermal conduction is included, reproducing both the observed morphology and the total X-ray luminosity very well. Finally, our results suggest that the two components of DEM L316 are not in physical interaction.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): conduction - hydrodynamics - methods: numerical - supernova remnants - Magellanic Clouds - X-rays: individual: DEM L316

Simbad objects: 8

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2020.09.18-17:36:06

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