A disc galaxy (or disk galaxy) is a galaxy characterized by a galactic disc. This is a flattened circular volume of stars that are mainly orbiting the galactic core in the same plane.[1] These galaxies may or may not include a central non-disc-like region (a galactic bulge).[2] They will typically have an orbiting mass of gas and dust in the same plane as the stars. Interactions with other nearby galaxies can perturb and stretch the galactic disk.
Disc galaxy types include:
- Spiral galaxies:
- Unbarred spiral galaxies: (types S, SA)
- Barred spiral galaxies: (type SB)
- Intermediate spiral galaxies: (type SAB)
- Lenticular galaxies: (types E8, S0, SA0, SB0, SAB0)
Galaxies that are not disc types include:
- Elliptical galaxies: (type dE)
- Irregular galaxies: (type dI)
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48 - Galaxy Morphology, Spiral Waves
Transcription
See also
References
- ^ "Disk Galaxies | COSMOS". astronomy.swin.edu.au.
- ^ "The Galactic Bulge". burro.case.edu.
This page was last edited on 29 September 2023, at 19:01