2018 Spring Semester Detail
The Journey of a Gemini Observer
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date. Feb. 28(Wednesday) * Speaker. Andre-Nicolas Chene (GEMINI Staff members) * Title. The Journey of a Gemini Observer * Abstract I have been a Gemini user for now
Network Cosmology : What I have learned from galaxy `Facebook`.
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date March 15 * Speaker Sungryong Hong (KIAS) * Title Network Cosmology : What I have learned from galaxy `Facebook`. * Abstract I have attempted to utilize network science tools for investigating topological
What is Nature Astronomy and how do I get published in it?
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date March 20(Tuesday) * Speaker Marios Karouzos (Nature Astronomy) * Title What is Nature Astronomy and how do I get published in it? * Abstract Nature Astronomy, launched in January 2017, is a
Chandra X-Ray Kinematics Study of Young Supernova Remnants
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date. March 22 * Speaker Sangwook Park (Univ. Texas Arlington) * Title. Chandra X-Ray Kinematics Study of Young Supernova Remnants * Abstract Supernova remnants are an excellent laboratory to
Formation of the First Galaxies and their Connection to Local Dwarfs
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date March 29 * Speaker Myoungwon Jeon (Kyung Hee Univ.) * Title Formation of the First Galaxies and their Connection to Local Dwarfs * Abstract One of the biggest challenges in modern cosmology
과학커뮤티케이터가 본 과학과 사회
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date April 5 * Speaker 이강환 (서대문자연사박물관) * Title 과학커뮤티케이터가 본 과학과 사회 * Abstract 과학이 점점 더 중요해지는 세상이다. 출판 시장의 어려움에도 불구하고 유일하게 과학책 분야만은 성장을 계속하고 있고, 능력 있는 국내
Molecular Gas Properties of HI Monsters
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date April 12 * Speaker Aeree Chung (Yonsei Univ.) * Title Molecular Gas Properties of HI Monsters * Abstract The cold gas reservoir surrounding present day massive galaxies like MW is generally insufficient
Introduction of Horizon Run 5 project and the other ongoing projects using numerical simulations
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date April 26 * Speaker Jihye Shin (KASI) * Title Introduction of Horizon Run 5 project and the other ongoing projects using numerical simulations * Abstract Horizon Run 5 will be the fifth
Magnetohydrodynamics of the circumstellar medium
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date May 3 * Speaker Allard Jan van Marle (UNIST) * Title Magnetohydrodynamics of the circumstellar medium * Abstract Stars shape the morphology of the medium around them through stellar winds. In this
Attack of the Lyman-Alpha Blobs: A Multi-Wavelength and Polarization Study
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date May 17 * Speaker Ann Zabludoff (Univ. Arizona) * Title Attack of the Lyman-Alpha Blobs: A Multi-Wavelength and Polarization Study * Abstract Lyman-alpha blobs are mysterious gas clouds in the distant
Upcoming Era in Numerical Galaxy Formation – New Possibilities and Challenges
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date May 24 * Speaker Ji-Hoon Kim (SNU) * Title Upcoming Era in Numerical Galaxy Formation – New Possibilities and Challenges * Abstract When experimenting with stars and galaxies is humanly impossible, numerical
Electromagnetic Radiation from the Gravitational Wave Source GW170817: Dawn of Multi-Messenger Astronomy
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date May 31 * Speaker Myungshin Im (Astronomy program, SNU) * Title Electromagnetic Radiation from the Gravitational Wave Source GW170817: Dawn of Multi-Messenger Astronomy * Abstract On August 17th 2017, for the first
Demographics of Stellar Populations in the Milky Way Galaxy
Colloquium Astronomy Colloquium (2018 Spring Semester) * Date June 7 * Speaker Deokkeun An (Ewha Womans Univ.) * Title Demographics of Stellar Populations in the Milky Way Galaxy * Abstract Recent large optical and near-infrared spectroscopic surveys have revolutionized our