Main Page: Difference between revisions
Jump to navigation
Jump to search
No edit summary |
No edit summary |
||
Line 18: | Line 18: | ||
{| class="wikitable" style="margin:auto" | {| class="wikitable" style="margin:auto" | ||
|- | |- | ||
| [[File:na2024.jpg|400px]] || [[File:coma.jpg| | | [[File:na2024.jpg|400px]] || [[File:coma.jpg|300px]] <br> Dark matter in the Coma Cluster region. The distribution of dark matter calculated based on this research (dark green cloud) is overlayed on an image of the Coma Cluster and more distant background galaxies taken by the Subaru Telescope. Strands of dark matter can be seen extending millions of light years. | ||
|- | |- | ||
|} | |} |
Revision as of 13:32, 22 May 2024
Welcome to Yonsei Observable UNiverse Group (YOUNG)
Publication in ADS
Google scholar
Research highlights