Discussion Overview
The discussion revolves around determining the mass of an Active Galactic Nucleus (AGN) given its luminosity in solar units. Participants explore the complexities involved in this estimation, particularly focusing on the limitations of using mass-luminosity relationships typically applied to main sequence stars.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Mathematical reasoning
Main Points Raised
- One participant questions the applicability of the mass-luminosity relationship for AGNs, noting that it is primarily relevant for main sequence stars.
- Another participant clarifies the context by confirming the luminosity is given in solar luminosities and specifies that they are discussing a galaxy rather than a star.
- A participant suggests that luminosity can be used to approximate the mass of a galaxy if distance and total luminosity are known, but emphasizes the complexity of this integration over angular size.
- It is proposed that knowing the distribution of stars in the galaxy could allow for an integration to estimate mass, assuming a main sequence star distribution, but acknowledges that this approach is complicated if the AGN is currently active.
Areas of Agreement / Disagreement
Participants express varying views on the methods for estimating mass from luminosity, with no consensus on a definitive approach or resolution of the complexities involved.
Contextual Notes
Participants note limitations such as the dependence on the distribution of stars and the complications introduced by an active central engine, which remain unresolved in the discussion.