SUMMARY
To determine the mass of an Active Galactic Nucleus (AGN) from a given luminosity of 12 trillion solar luminosities, one cannot rely solely on the mass-luminosity relationship applicable to main sequence stars. Instead, integrating the luminosity over the galaxy's angular size is necessary, although this method is complex and often avoided for simpler estimation techniques. A more accurate approach involves knowing the distribution of stars within the galaxy, particularly using the initial mass function to normalize the total luminosity. This results in a linear relationship between luminosity and mass, with a proportionality constant ranging from 1 to 10.
PREREQUISITES
- Understanding of Active Galactic Nuclei (AGN)
- Familiarity with luminosity and its measurement in solar units
- Knowledge of stellar distribution and initial mass function
- Basic principles of integrating functions over angular sizes
NEXT STEPS
- Research methods for integrating luminosity over angular size in astrophysics
- Study the initial mass function and its application in galaxy mass estimation
- Explore the relationship between luminosity and mass in different types of galaxies
- Investigate the effects of an active central engine on mass estimation of AGNs
USEFUL FOR
Astronomers, astrophysicists, and students studying galaxy formation and dynamics, particularly those interested in the mass estimation of Active Galactic Nuclei.