Kavli Affiliate: Jing Wang | First 5 Authors: Xiao Li, Xiao Li, , , | Summary: While massive quiescent galaxies are known to be poor in atomic hydrogen (HI), their true HI content remains poorly constrained due to the limited sensitivity and morphological biases of existing surveys. We present deep HI observations using the Five-hundred-meter […]
Continue.. What is the True HI Gas Content in Massive Quiescent Galaxies in the Local Universe?