Discussion Overview
The discussion centers around the classification of black holes, specifically whether Sagittarius A* is a quasar or a blazar, and the mechanisms by which jets emitted by black holes can be studied. It also touches on the effects of orbital motion of gas around black holes on observed spectra, with a focus on the case of M87.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Homework-related
Main Points Raised
- Some participants assert that black holes themselves are neither quasars nor blazars, as they do not emit radiation directly, but rather the surrounding accretion disc does.
- Others explain that quasars and blazars are types of active galactic nuclei (AGNs) powered by black holes, with blazars being particularly bright due to their jets pointing towards Earth.
- One participant inquires about the methods used to study the jets of black holes.
- A new participant poses a question regarding the influence of the orbital motion of gas around the black hole in M87 on its observed spectrum, seeking clarification on the relationship between motion and spectral shifts.
- Another participant agrees with the notion that the orbital motion affects the spectrum, elaborating on the redshift and blueshift phenomena due to the gas's motion towards and away from the observer.
- Further discussion explores the implications of excluding specific information about the gas's motion and how that might affect the understanding of spectral oscillations.
Areas of Agreement / Disagreement
Participants express differing views on the classification of black holes in relation to quasars and blazars, and while there is some agreement on the effects of gas motion on spectral observations, the discussion remains unresolved regarding the broader implications and specific mechanisms involved.
Contextual Notes
Limitations include assumptions about the nature of black holes and the definitions of AGNs, as well as the complexity of the interactions between gas motion and observed spectra, which are not fully explored in the discussion.
Who May Find This Useful
This discussion may be of interest to those studying astrophysics, particularly in the areas of black hole physics, active galactic nuclei, and spectral analysis of astronomical objects.