Open Access
Table 2.
Ranking of feedback mechanisms w.r.t. their impact on the global morphology of the gas fields at z ≲ 1.5 and z ≳ 1.5 (first and second number).
| T | P | ngas | nHI | nH2 | Z | |
|---|---|---|---|---|---|---|
| X-ray heating | 2–2 | 3–2 | 4–2 | 2–2 | 4–2 | 3–4 |
| Jets | 1–1 | 2–3 | 3–3 | 4–3 | 3–3 | 1–2 |
| AGN winds | 4–4 | 1–4 | 2–4 | 3–4 | 2–4 | 4–3 |
| Stellar feedback | 3–3 | 1–1 | 1–1 | 1–1 | 1–1 | 2–1 |
Notes. For instance, the morphology of the T-field at z ≲ 1.5 is mostly affected by jets, then by X-ray heating, stellar feedback, and AGN winds in this order.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.