A5064448595- Astronomy and Astrophysical Research
- Galaxies: Formation, Evolution, Phenomena
- Astronomical Observations and Instrumentation
- Radio Astronomy Observations and Technology
- Cosmology and Gravitation Theories
- Stellar, planetary, and galactic studies
- Solar and Space Plasma Dynamics
- Computational Physics and Python Applications
International Centre for Radio Astronomy Research
2024
The University of Western Australia
2024
ABSTRACT We introduce version 2.0 of the shark semi-analytic model galaxy formation after many improvements to physics included. The most significant being (i) a describing exchange angular momentum (AM) between interstellar medium and stars; (ii) new active galactic nuclei feedback which has two modes, wind jet mode, with mode tied energy production; (iii) tracking development black hole (BH) spins; (iv) more sophisticated modelling environmental effects on satellite galaxies; (v) automatic...
We introduce version 2.0 of the SHARK semi-analytic model galaxy formation after many improvements to physics included. The most significant being: (i) a describing exchange angular momentum (AM) between interstellar medium and stars; (ii) new active galactic nuclei feedback which has two modes, wind jet mode, with mode tied energy production; (iii) tracking development black hole (BH) spins; (iv) more sophisticated modelling environmental effects on satellite galaxies; (v) automatic...
ABSTRACT We present a model of radio continuum emission associated with star formation (SF) and active galactic nuclei (AGNs) implemented in the Shark semi-analytic galaxy formation. SF includes free-free synchrotron emission, which depend on free-electron density rate core-collapse supernovae minor contribution from supernova remnants, respectively. AGN is modelled based jet production rate, depends black hole mass, accretion spin, self-absorption. reproduces luminosity functions (RLFs) at...