125 citations
- Korea Astronomy and Space Science InstituteKR6 papers
- Sejong UniversityKR5 papers
- Gyeongguk National UniversityKR3 papers
- Korea Advanced Institute of Science and TechnologyKR3 papers
- California Institute of TechnologyUS2 papers
- CEA Paris-SaclayFR2 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2 papers
- Consejo Superior de Investigaciones CientíficasES2 papers
- Hampton UniversityUS2 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT2 papers
- Johns Hopkins UniversityUS2 papers
- Kharkiv Institute of Physics and TechnologyUA2 papers
5 papers · 1 filter
A study of the Correlation of Arrival Directions of UHECRs with the Large Scale Structure of the Universe
Dongsu Ryu, Hyesung Kang, Santabrata Das
Ultrahigh energy cosmic rays (UHECRs) are believed to originate from astrophysical sources, which should trace the large scale structure (LSS) of the universe. On the other hand, t…
Probing the Intermediate-Age Globular Clusters in NGC 5128 from Ultraviolet Observations
Soo-Chang Rey, Sangmo T. Sohn, Michael A. Beasley +23
We explore the age distribution of the globular cluster (GC) system of the nearby elliptical galaxy NGC 5128 using ultraviolet (UV) photometry from Galaxy Evolution Explorer (GALEX…
An Ultraviolet Study of Star-Forming Regions in M31
Yongbeom Kang, Luciana Bianchi, Soo-Chang Rey
We present a comprehensive study of star-forming (SF) regions in the nearest large spiral galaxy M31. We use GALEX far-UV (1344-1786 Å, FUV) and near-UV (1771-2831 Å, NUV) imaging…
Triggered Star Formation in a Double Shell near W51A
Miju Kang, John H. Bieging, Craig A. Kulesa +1
We present Heinrich Hertz Telescope CO observations of the shell structure near the active star-forming complex W51A to investigate the process of star formation triggered by the e…
Simulations of Electron Magnetohydrodynamic Turbulence
Jungyeon Cho, A. Lazarian
We present numerical simulations of electron magnetohydrodynamic (EMHD) and electron reduced MHD (ERMHD) turbulence. Comparing scaling relations, we find that both EMHD and ERMHD t…