2009MNRAS.395..351T


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.21CEST16:04:51

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

goto Full paper

goto View the reference in ADS

Number of rows : 8

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 5758 1
2 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14989 1
3 DEM L 316b SNR 05 47 00.00 -69 43 00.0           ~ 23 0
4 SNR B0547-69.7 SNR 05 47 17.5 -69 41 38           ~ 92 1
5 DEM L 316a SNR 05 47 21.0 -69 41 25           ~ 27 0
6 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 831 2
7 SNR G039.7-02.0 SNR 19 12 20 +04 55.0           ~ 315 1
8 SNR G053.6-02.2 SNR 19 38.8 +17 14           ~ 137 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2009MNRAS.395..351T and select 'bookmark this link' or equivalent in the popup menu


2020.10.21-16:04:51

© Université de Strasbourg/CNRS

    • Contact