Dark Matter in the Central Region of NGC 3256
We investigated the central mass distribution of the luminous infrared galaxy NGC 3256 at a distance of 35 Mpc by using CO(1-0) observations of the Atacama Large Millimeter and sub-millimeter Array (ALMA) and near-IR data of the Two Micron Sky Survey (2MASS). We found that there is a huge amount of...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Published: |
Penerbit Universiti Kebangsaan Malaysia
2018
|
| Subjects: |