Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Seoul National University, Seoul, Korea
Department of Physics and Astronomy, Seoul National University, Seoul, Korea
SNU
Seoul National University, Korea
Astronomy program, SEES, Seoul National University, Korea
California, University, Berkeley
Astronomy Program, SEES, Seoul National University, Seoul 151-747, Korea
Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea Univ., Berkeley; Seoul National Univ., Republic of Korea
Department of Astronomy, Seoul National University, Korea
Astronomy Program, SEES, Seoul National University, Seoul 151-742, Korea
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Seoul National Univ., Seoul, Korea
NASA. Goddard Space Flight Center, Greenbelt, MD, US
Astronomy Program, SEES, Seoul National University, Seoul 151-742, South Korea National University, Korea, Republic of of Physics and Astronomy, Seoul National University, Seoul 151-742, Republic of Korea of Astronomy, Seoul National University, Seoul 151-742, Korea
Seoul National Univ., Korea, Republic of
Astronomy Program, SEES, Seoul National University, Seoul 151-742, South Korea; Visiting Professor, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan. Department, Seoul National University
Seoul National University SRAO
Koo
Seoul National University
Department of Physics and Astronomy, Seoul National University, Seoul 151-747, South Korea
Seoul National University, Seoul, Korea, South
National Astronomical Observatory; Seoul National University, Republic of Korea
SNU, Korea
1.4GHz-Band Radio Interferences at Seoul Radio Astronomical Observatory
12CO 4-3 and [CI] 1-0 at the centers of NGC 4945 and Circinus
2MASS near-infrared images of RCW 103: A young SNR in a dense medium
A 21 cm Spectral and Continuum Study of IC 443 Using the Very Large Array and the Arecibo Telescope
A Design Study of the 400MHz Wide-Band Digital Autocorrelation Spectrometer
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