All Outputs (3)

158 μm emission as an indicator of galaxy star formation rate (2023)
Journal Article
Liang, L., Feldmann, R., Murray, N., Narayanan, D., Hayward, C. C., Angles-Alcázar, D., …Hopkins, P. F. (2024). 158 μm emission as an indicator of galaxy star formation rate. Monthly notices of the Royal Astronomical Society, 528(1), 499-541. https://doi.org/10.1093/mnras/stad3792

Observations of local star-forming galaxies (SFGs) show a tight correlation between their singly ionized carbon line luminosity () and star formation rate (SFR), suggesting that may be a useful SFR tracer for galaxies. Some other galaxy populations,... Read More about 158 μm emission as an indicator of galaxy star formation rate.

Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations (2023)
Journal Article
Mercedes-Feliz, J., Anglés-Alcázar, D., Hayward, C. C., Cochrane, R. K., Terrazas, B. A., Wellons, S., …Kereš, D. (2023). Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations. Monthly notices of the Royal Astronomical Society, 524(3), 3446-3463. https://doi.org/10.1093/mnras/stad2079

Negative feedback from accreting supermassive black holes is considered crucial in suppressing star formation and quenching massive galaxies. However, several models and observations suggest that black hole feedback may have a positive effect, trigge... Read More about Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations.

Hydrodynamic simulations of the disc of gas around supermassive black holes (HDGAS) -I. Molecular gas dynamics (2023)
Journal Article
Raouf, M., Viti, S., García-Burillo, S., Richings, A. J., Schaye, J., Bemis, A., …Holdship, J. (2023). Hydrodynamic simulations of the disc of gas around supermassive black holes (HDGAS) -I. Molecular gas dynamics. Monthly notices of the Royal Astronomical Society, 524(1), 786-800. https://doi.org/10.1093/mnras/stad1957

We present hydrodynamic simulations of the interstellar medium (ISM) within the circumnuclear disc (CND) of a typical active galactic nucleus (AGN)-dominated galaxy influenced by mechanical feedback from an AGN. The simulations are coupled with the C... Read More about Hydrodynamic simulations of the disc of gas around supermassive black holes (HDGAS) -I. Molecular gas dynamics.