Research Highlights
Identifying galaxy groups and clusters in the high-z universe
12 6月 2020Identifying galaxy groups and clusters in the high-z universe 12 Jun 2020 Galaxies are not distributed at random. Rather, they are found to be clustered, with half...
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Bars enhance the central star formation and gas inflow in nearby galaxies
07 6月 2020Bars enhance the central star formation and gas inflow in nearby galaxies 07 Jun 2020 Two thirds of spiral galaxies in the local Universe are observed to have a ba...
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PolarLight results featured on the cover of Nature Astronomy
11 5月 2020PolarLight results featured on the cover of Nature Astronomy 11 May 2020 On May 11, Professor Hua Feng and collaborators reported in Nature Astronomy a re-detecti...
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Estimating stellar dust attenuation from galactic spectra
24 3月 2020Estimating stellar dust attenuation from galactic spectra 24 3月 2020 The observed spectrum of a galaxy is a combination of several components: a continuum, absorp...
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Recovering star formation histories of low-mass galaxies
20 3月 2020Recovering star formation histories of low-mass galaxies 20 3月 2020 Characterizing the star formation history (SFH) of galaxies is an important step toward a full...
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Searching for Wolf-Rayet Regions of Massive Stars in Galaxies
15 3月 2020Searching for Wolf-Rayet Regions of Massive Stars in Galaxies 15 3月 2020 Wolf-Rayet (WR) galaxies are a rare population of galaxies that host living high-mass sta...
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