At z≈0.43, massive star-forming galaxies host 3x more O VI in their inner halos than quiescent galaxies of the same stellar mass, with an O VI mass offset of ~1.5 dex, contradicting the virial-thermometer prediction.
L., Faerman, Y., Berg, T
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The GOLIATH Survey: OVI Absorption Reveals CGM Evolution through the Starburst-to-Quiescent Transition in Massive Galaxies
At z≈0.43, massive star-forming galaxies host 3x more O VI in their inner halos than quiescent galaxies of the same stellar mass, with an O VI mass offset of ~1.5 dex, contradicting the virial-thermometer prediction.