访问学者
Past Visiting Scholars
| Visitor | Period of stay | Research interests | |
|---|---|---|---|
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Piero Madau University of California Santa Cruz |
15 Oct 2018 to 29 Oct 2018 | Dr. Madau has pioneered many areas that later developed into staples of standard modern cosmology. His tools range from pencil-and-paper to the most ambitious cosmological N-body and hydrodynamical simulations. |
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Scott Tremaine Institute for Advanced Study, Princeton |
8 Oct 2018 to 11 Oct 2018 | comets, the solar system, exoplanets, star clusters, black holes, galaxies, and cosmology |
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Alberto Sesana University of Birmingham |
7 Oct 2018 to 25 Oct 2018 | Gravitational waves; Massive black hole (binaries); Stellar dynamics, dense stellar systems; Hyper–velocity stars and the nature and environment of SgrA∗; Gas dynamics and accretion theory; Structure formation and galaxy evolution. |
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Cristina Romero-Canizales Nucleo de Astronomia, Universidad Diego Portales, Chile |
23 Sep 2018 to 21 Oct 2018 | Radio/mm studies of interacting/merging galaxies Galaxy evolution and star formation Tidal Disruption Events at high angular resolution Astronomical masers |
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Emiko Hiyama Kyushu Univeristy |
9 Sep 2018 to 1 Oct 2018 | Particle/Nuclear/Cosmic ray/Astro physics |
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Sharon Wang Carnegie-DTM |
5 Sep 2018 | current research focuses on improving the RV precision |
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Boaz Katz Weizmann Institute of Science |
7 Aug 2018 to 15 Aug 2018 |
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Claudio Ricci Universidad Diego Portales |
6 Jul 2018 to 2 Aug 2018 | Active Galactic Nuclei, X-ray astronomy |
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Li Aigen University of Missouri |
28 Jun 2018 to 2 Jul 2018 | Interstellar Dust Dust Disks around Young Stars Dust Envelopes around Evolved Stars Physics and Chemistry of Comets Infrared Galaxies Active Galactic Nuclei Gamma-Ray Bursts Light Scattering by Small Particles |
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Jianhui LIAN University of Portsmouth |
25 Jun 2018 | My current research interest mainly lies in understanding the chemical evolution of external galaxies and our Milky Way from both an observational and an theoretical angle. Besides, I am also interested in the star formation history of galaxies, especially the quenching process, and galaxy structure from deep and high spatial resolution photometry. |
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