An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
Research output: Contribution to journal › Journal article › Research › peer-review
Using our measurements of the H alpha emission line flux originating in the cool (T similar to 10(4) K) gas that populates the halos of galaxies, we build a joint model to describe the mass of the cool circumgalactic medium (CGM) as a function of galactic stellar mass (10(9.5)
| Original language | English |
|---|---|
| Article number | 101 |
| Journal | Astrophysical Journal |
| Volume | 916 |
| Issue number | 2 |
| Number of pages | 15 |
| ISSN | 0004-637X |
| DOIs | |
| Publication status | Published - 3 Aug 2021 |
- STAR-FORMATION HISTORIES, LYMAN-ALPHA EMISSION, GAS DEPLETION TIME, COSMOLOGICAL SIMULATIONS, PHYSICAL-PROPERTIES, MOLECULAR GAS, GALAXY, ABSORPTION, EVOLUTION, MODEL
Research areas
Links
- https://arxiv.org/pdf/2104.12777.pdf
Submitted manuscript
ID: 275990688