Discussion Overview
The discussion centers on the likelihood of different types of galaxy collisions, specifically whether two elliptical galaxies are more likely to collide and form two spiral galaxies, or if two spiral galaxies are more likely to collide and form two elliptical galaxies. The scope includes theoretical considerations and interpretations of simulation results.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- Some participants suggest that simulations indicate two spiral galaxies colliding will likely produce an elliptical galaxy.
- One participant describes the process of two spirals colliding, proposing that the collision results in gas being thrown in random directions, leading to the formation of an elliptical galaxy.
- Another participant argues that a complex structure like a spiral disk can only evolve after a long period of stability, implying that major disturbances lead to elliptical galaxies, but with enough time, these could evolve into spirals.
- A different viewpoint mentions that the disk structure is not inherently complex, and that density waves within the disk contribute to the formation of spiral arms, which may misrepresent the density of star formation in the galaxy.
Areas of Agreement / Disagreement
Participants express differing views on the outcomes of galaxy collisions, with no consensus reached on which scenario is more likely. The discussion remains unresolved regarding the specific processes and outcomes of these collisions.
Contextual Notes
Some assumptions about the stability of galaxy structures and the conditions necessary for the evolution of spiral galaxies are not fully explored. The discussion also reflects varying interpretations of simulation data and theoretical models.