Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
KAO / Trao, Cfa
Korea Astronomy and Space Science Institute
University of California, Berkeley, CA, US
Korea Astronomy Observatory, Taeduk Radio Astronomy Observatory, Whaam-dong 61-1, Yusong-gu, Taejon, 305-348, Korea
Korea Astronomy & Space Science Institute, Daejeon 305-348, Korea College Radio Astronomy Observatory, Amherst, MA
Korea Astronomy and Space Science, Republic of Korea
Korea Astronomy Observatory, Taejon 305-348, Korea
Korea Astronomy Observatory, Korea
Korea Astronomy Observatory / Taeduk Radio Astronomy Observatory, Hwaam-dong 61-1, Yusong-gu, Taejon, 305-348, Korea
Korea Astronomy Observatory, Taeduk Radio Astronomy Observatory, Taejon, Korea
University of Florida & FCRAO
Taeduk Radio Astronomical Observatory, Korea Astronomy Observatory, Korea
Korea Astronomy Observatory, Taeduk Radio Astronomy Observatory, Hwaam-dong 61-1, Yuseong-gu, Daejeon 305-348, Republic of Korea.
Korea Astronomy Observatory, Taeduk Radio Astronomy Observatory, Hwaam-dong 61-1, Yuseong-gu, Daejeon, 305-348, South Korea
Korea Astronomy Observatory / Taeduk Radio Astronomy Observatory, Daejon, Korea
Seoul National Univ., Seoul, Korea
Taeduk Radio Astronomy Observatory, San 36-1, Whaam-Dong, Youseong-Gu, Taejeon 305-348, Korea.
Korea Astronomy and Space Science Institute, Taeduk Radio Astronomy Observatory, Daejeon 305-348, Korea
Korea Astronomy and Space Science Institute, International Center for Astrophysics, Daejeon 305-348, Korea
Korea Astronomy Observatory, 61-1, Hwaam, Yuseong, Daejeon 305-348, South Korea
Five College Radio Observatory, Massachusetts Univ., Amherst, MA, US
A CO Line and Infrared Continuum Study of the Active Star-Forming Complex W51
A Fast Reduction Method of Survey Data in Radio Astronomy
A Highly Disturbed Molecular Cloud S287: I. CO Observations and Kinematics
A molecular cloud complex above the galactic plane.. I. Extended CO observations of the NGC 281 region
A Molecular Line Survey of W3(OH) and W3 IRS 5 from 84.7 to 115.6 GHz: Observational Data and Analyses
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