Hee-Jae Lee
Chungbuk National University
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Publication
Featured researches published by Hee-Jae Lee.
Journal of Astronomy and Space Sciences | 2016
Jin Choi; Jung Hyun Jo; Myung-Jin Kim; Dong-Goo Roh; Sun-Youp Park; Hee-Jae Lee; Maru Park; Young-Jun Choi; Hong-Suh Yim; Young-Ho Bae; Youngsik Park; Sungki Cho; Hong-Kyu Moon; Eun-Jung Choi; Hyun-Jung Jang; Jang-Hyun Park
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The Astrophysical Journal | 2017
Chan-Kao Chang; Hsing-Wen Lin; Wing-Huen Ip; Z.-Y. Lin; T. Kupfer; Thomas A. Prince; Quan-Zhi Ye; Russ R. Laher; Hee-Jae Lee; Hong-Kyu Moon
(144977) 2005 EC127 is an V-/A-type inner-main-belt asteroid with a diameter of 0.6 +- 0.1 km. Asteroids of this size are believed to have rubble-pile structure, and, therefore, cannot have a rotation period shorter than 2.2 hours. However, our measurements show that asteroid 2005 EC127 completes one rotation in 1.65 +- 0.01 hours with a peak-to-peak light-curve variation of ~0.5 mag. Therefore, this asteroid is identified as a large super-fast rotator. Either a rubble-pile asteroid with a bulk density of ~6 g cm^-3 or an asteroid with an internal cohesion of 47 +- 30 Pa can explain 2005 EC127. However, the scenario of high bulk density is very unlikely for asteroids. To date, only six large super-fast rotators, including 2005 EC127, have been reported, and this number is very small when compared with the much more numerous fast rotators. We also note that none of the six reported large SFRs are classified as C-type asteroids.
Journal of the Korean Astronomical Society | 2017
Hee-Jae Lee; Hong-Kyu Moon; Myung-Jin Kim; Chun-Hwey Kim; Josef Durech; Young-Jun Choi; Young-Seok Oh; Jintae Park; Dong-Goo Roh; Hong-Suh Yim; Sang-Mok Cha; Yong Seok Lee
We conduct BVRI and R band photometric observations of asteroid (5247) Krylov from January 2016 to April 2016 for 51 nights using the Korea Microlensing Telescope Network (KMTNet). The color indices of (5247) Krylov at the light curve maxima are determined as B − V = 0.841± 0.035, V −R = 0.418± 0.031, and V − I = 0.871± 0.031 where the phase angle is 14.1. They are acquired after the standardization of BVRI instrumental measurements using the ensemble normalization technique. Based on the color indices, (5247) Krylov is classified as a S-type asteroid. Double periods, that is, a primary period P1 = 82.188 ± 0.013h and a secondary period P2 = 67.13 ± 0.20 h are identified from period searches of its R band light curve. The light curve phases with P1 and this indicate that it is a typical Non-Principal Axis (NPA) asteroid. We discuss the possible causes of its NPA rotation.
KIISE Transactions on Computing Practices | 2017
Jae-Keun Yeom; Jung-Lok Yu; Hong-Suh Yim; Myung-Jin Kim; Jintae Park; Hee-Jae Lee; Hong-Kyu Moon; Young-Jun Choi; Dong-Goo Roh; Young-Seok Oh; Young-Ho Bae
한국천문학회보 | 2016
Dong-Goo Roh; Hong-Kyu Moon; Min-Su Shin; Hee-Jae Lee; Myung-Jin Kim
한국천문학회보 | 2016
Hong-Suh Yim; Myung-Jin Kim; Dong-Goo Roh; Jintae Park; Hong-Kyu Moon; Young-Jun Choi; Young-Ho Bae; Hee-Jae Lee; Young-Seok Oh
한국천문학회보 | 2016
Dong-Goo Roh; Hong-Kyu Moon; Myung-Jin Kim; Jintae Park; Young-Jun Choi; Hong-Suh Yim; Hee-Jae Lee; Young-Suk Oh
한국천문학회보 | 2016
Hee-Jae Lee; Myung-Jin Kim; Hong-Kyu Moon; Jintae Park; Chun-Hwey Kim; Young-Jun Choi; Hong-Suh Yim; Dong-Goo Roh; Young-Seok Oh
한국천문학회보 | 2016
Myung-Jin Kim; Hong-Kyu Moon; Young-Jun Choi; Hong-Suh Yim; Jintae Park; Dong-Goo Roh; Hee-Jae Lee; Young-Seok Oh
한국천문학회보 | 2016
Hong-Kyu Moon; Myung-Jin Kim; Dong-Goo Roh; Jintae Park; Hong-Suh Yim; Young-Jun Choi; Young-Ho Bae; Hee-Jae Lee; Young-Seok Oh