SIMBAD references

2015MNRAS.450.2799C - Mon. Not. R. Astron. Soc., 450, 2799-2811 (2015/July-1)

The soft and hard X-rays thermal emission from star cluster winds with a supernova explosion.

CASTELLANOS-RAMIREZ A., RODRIGUEZ-GONZALEZ A., ESQUIVEL A., TOLEDO-ROY J.C., OLIVARES J. and VELAZQUEZ P.F.

Abstract (from CDS):

Massive young star clusters contain dozens or hundreds of massive stars that inject mechanical energy in the form of winds and supernova explosions, producing an outflow which expands into their surrounding medium, shocking it and forming structures called superbubbles. The regions of shocked material can have temperatures in excess of 106 K, and emit mainly in thermal X-rays (soft and hard). This X-ray emission is strongly affected by the action of thermal conduction, as well as by the metallicity of the material injected by the massive stars. We present three-dimensional numerical simulations exploring these two effects, metallicity of the stellar winds and supernova explosions, as well as thermal conduction.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): stars: winds, outflows - ISM: bubbles - open clusters and associations: general - galaxies: star clusters: general - X-rays: ISM

Simbad objects: 8

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2015MNRAS.450.2799C and select 'bookmark this link' or equivalent in the popup menu