Astrophysics (Index)About

disk galaxy

(circular, relatively flat galaxy such as a spiral galaxy)

Disk galaxy is a term for disk-shaped galaxies (e.g., as opposed to elliptical galaxies), including spiral galaxies, and including galaxies that are generally disk-shaped, even if they have a bulge, such as lenticular galaxies. The term disk refers to the galaxy's disk-like feature, often not intended to include the protrusions of any bulge. Some observation and analysis suggests the disks of galaxies often can be distinguished to be overlaid disks of distinctive stars, each with its distinctive gas, dust, and kinematic characteristics. In the case of the Milky Way, a thick disk (of thick disk stars) has within it, a thin disk (of thin disk stars), the latter apparently younger, the result of more recent star formation.


(galaxy type)
Further reading:
https://en.wikipedia.org/wiki/Disc_galaxy
https://en.wikipedia.org/wiki/Thick_disk
https://en.wikipedia.org/wiki/Thin_disk
https://astronomy.swin.edu.au/cosmos/d/Disk+Galaxies

Referenced by pages:
alpha-enhanced
bulge
corotation resonance
disk
epicycle
galactic disk
galactic plane
galactic tide
galaxy
galaxy classification
globular cluster (GC)
gravitational instability (GI)
heating
lenticular galaxy (S0)
Lindblad resonance
Lindblad torque
metallicity gradient
Milky Way (MW)
peculiar galaxy (p)
radial mixing
satellite plane problem
spiral galaxy
stellar dynamics
thick disk
thin disk
Toomre Q parameter (Q)
warp

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