Research Highlights
通过自行推断银河系核球中RR Lyrae变星的旋转特性
26 8月 2020通过自行推断银河系核球中RR Lyrae变星的旋转特性 26 8月 2020 RR Lyrae变星是一类贫金属、氦核燃烧的水平支巨星，通常年龄在10 Gyr以上。它们的周光关系使得我们能更精确地确...
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“极光计划”成果登上《自然·天文》封面
11 5月 2020“极光计划”成果登上《自然·天文》封面 11 5月 2020 5月11日，清华大学天文系教授冯骅课题组与合作者在《自然·天文》杂志发表封面文章，报道了清华大学主导的空间天文项目“极...
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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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Relating structure of dark halos to their assembly and environment
12 3月 2020Relating 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...
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