Estimating stellar dust attenuation from galactic spectra
Estimating 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...
阅读更多...Estimating 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...
阅读更多...Recovering 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...
阅读更多...Searching 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...
阅读更多...LHS 1815b: The First Thick-Disk Planet Detected By TESS 12 3月 2020 To date, more than 4000 exoplanets have been detected, but few of them have been claimed to be ...
阅读更多...Relating structure of dark halos to their assembly and environment 12 3月 2020 Dark matter halos are the building blocks of the cosmic large-scale structures and t...
阅读更多...Tsinghua Vice President Xue Qikun visits DoA 07 3月 2020 In the morning of March 6, 2020, Tsinghua University Vice President XUE Qikun visited the Department of As...
阅读更多...Machine learning recovers H II morphology during reionization 01 3月 2020 The epoch of reionization (EoR) is a unique period of time in cosmic evolution, during wh...
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