Discussion Overview
The discussion centers on the measurement and interpretation of redshifts in quasars, questioning whether current methodologies might be flawed. Participants explore the implications of these measurements for theories such as the Big Bang and the expansion of the universe, while also considering alternative explanations for quasar behavior.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- Some participants question why quasars do not exhibit redshift, suggesting that all measurements cannot be incorrect and speculating on the validity of the Big Bang theory.
- Others assert that quasars do have measured redshifts and critique the interpretation of recent studies, emphasizing the complexity of measurements and potential biases in data interpretation.
- One participant expresses skepticism about the prevailing view of quasars being at their redshift distances, citing Arp's interpretation as a plausible alternative, while also critiquing Arp's theoretical framework.
- Another participant provides links to studies claiming evidence of quasar host galaxies at corresponding redshifts, challenging the notion that these hosts are merely artifacts.
- Some participants highlight the need for careful analysis of the relationship between quasars and their host galaxies, noting that the apparent redshift of quasars may change over time.
- There is a call for statistical analysis to support claims regarding the relationship between quasars and their host galaxies, indicating a desire for more rigorous evidence.
Areas of Agreement / Disagreement
Participants express a range of views, with no consensus reached on the interpretation of quasar redshifts or the validity of competing theories. Disagreement persists regarding the implications of recent studies and the interpretations of quasar-host relationships.
Contextual Notes
Participants note limitations in the current understanding of quasar measurements, including potential biases in data interpretation and the complexity of distinguishing between different causes of optical variations in quasars.