Abstract
SPT0311-58, a system of two interacting galaxies in the Epoch of
Reionization, exists in one of the rarest, most massive dark matter
halos theoretically possible in that era. Studying the interstellar
medium (ISM) in these galaxies can illuminate the process of galaxy
formation in the early Universe. In this work, we explore the multiphase
ISM in this system, using ALMA observations of the [C ii] 158, [O i] 146, [N ii] 122, and [O iii]
88 fine-structure lines and dust continuum. We find wide variations in
line ratios between the eastern and western galaxies, as well as across
the western galaxy.
| Original language | English |
|---|---|
| Article number | 87 |
| Journal | Astrophysical Journal |
| Volume | 949 |
| Issue number | 2 |
| Number of pages | 9 |
| ISSN | 0004-637X |
| DOIs | |
| Publication status | Published - 2023 |
Keywords
- Interstellar medium
- High-redshift galaxies