X-ray emission from hot gas in galaxy groups and clusters in simba
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DOI: 10.1093/mnras/staa2394
Abstract: We examine X-ray scaling relations for massive halos ($M_{500}>10^{12.3}M_\odot$) in the Simba galaxy formation simulation. The X-ray weighted luminosity, $L_X$ vs. $M_{500}$ has power-law slopes $\approx\frac{5}{3}$ and $\approx\frac{8}{3}$ above and below $10^{13.5} M_{\odot}$, deviating from… read more here.
Keywords: halos; ray; core; galaxy ... See more keywords