2015MNRAS.450.2799C

Query : 2015MNRAS.450.2799C

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

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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 - 2026 		#notes
1 LHA 120-N 185 EmO 04 53 58.9 -70 00 53           ~ 40 0
2 LHA 120-N 186 EmO 04 59 45.5 -70 09 45           ~ 40 0
3 LHA 120-N 44 EmO 05 22 06.9 -67 56 46           ~ 211 1
4 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
5 LHA 120-N 70 HII 05 43 17.5 -67 50 48           ~ 85 0
6 NAME Rosette Nebula HII 06 32 26.76 +04 47 37.1           ~ 522 1
7 NGC 3603 OpC 11 14 57.9 -61 14 32           ~ 1136 1
8 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1700 0

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