MUSE surveys intermediate-redshift galaxies

We quantify the stellar rotation of galaxies by computing the {lambda}R parameter, a proxy for the stellar angular momentum in a sample of 106 intermediate-redshift galaxies (0.1本研究通过计算λ_R参数（lambda R），对106个中等红移星系（0.1）样本的恒星自转进行定量表征，该参数可作为恒星角动量的代理变量