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The Evolution of the Galaxy Cluster Luminosity-Temperature Relation

Megan C. Novicki·Manuela Sornig·J. Patrick Henry
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Abstract

We analyzed the luminosity-temperature (L-T) relation for 2 samples of galaxy clusters which have all been observed by the ASCA satellite. We used 32 high redshift clusters (0.3<z<0.6), 53 low redshift clusters (z<0.3), and also the combination of the low and high redshift datasets. We assumed a power law relation between the bolometric luminosity of the galaxy cluster and its integrated temperature and redshift (L_{bol,44}=C*T^alpha*(1+z)^A). The results are consistent, independent of cosmology, with previous estimates of L$\sim$T$^3$ found by other authors. We observed weak or zero evolution.

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Megan C. Novicki, Manuela Sornig, J. Patrick Henry. 2002-08-27. The Evolution of the Galaxy Cluster Luminosity-Temperature Relation. https://doi.org/10.1086/344162

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