Astrophysics (Index)About

spiral galaxy

(flat galaxy with spiraling arms)

A spiral galaxy is a disk galaxy that has spiral arms, one of three galaxy classes described by Edwin Hubble along with elliptical galaxies and lenticular galaxies. The galaxy classification designations for spiral galaxies are SA or SB (or SAB for something between) followed by a letter, a, b, c or d, indicating how tight are the arms. SB is for barred, i.e., a barred galaxy, a spiral galaxy whose center appears like a bar between two opposing arms rather than just a circular mass of stars. Spiral galaxies are generally younger than elliptical galaxies with more interstellar gas and dust, and are generally forming stars. There is a correlation between color and spiral/disk versus elliptical: that flat galaxies tend to be blue, indicating early stars and star formation, and elliptical galaxies tend to be red. However red spiral galaxies do exist.

The dynamics that produces the galaxy's spiral structure (i.e., the spiral arms) is not immediately apparent: if the arm structure simply consisted of the position of the stars as they orbit around the galaxy, the inner stars getting around quicker than the outer stars would make the arms wrap tighter with time, and there would be more tightly-wrapped galaxies than are seen in surveys. A classic theory consists of spiral density waves (of higher-density intergalactic medium) feeding a visible spiral wave of star formation. Many of the created stars will be bright but short-lived, so a traveling line of star formation will show as a line of brightness, a spiral arm. N-body simulations have produced spiral structures, but under varying assumptions.

The stars' orbits are not simple circles, and probably not ellipses, and efforts to characterize the orbits in a useful way include breaking each into an epicyclic frequency (toward and away from the center) and vertical oscillation frequency (up and down from the plane).

Example spiral galaxies:

The Magellanic clouds have been considered irregular but are now sometimes cited as single-armed spiral galaxies, termed Magellanic spiral galaxies. An anemic galaxy is a spiral galaxy where the spirals and the portions between them show less contrast, i.e., like lenticular galaxies but with a visible spiral pattern. A flocculent spiral galaxy is one where the spiral arms are not continuous, but patches of brightness.


(galaxy type)
Further reading:
http://en.wikipedia.org/wiki/Spiral_galaxy
http://en.wikipedia.org/wiki/Barred_spiral_galaxy
http://en.wikipedia.org/wiki/Anemic_galaxy
http://en.wikipedia.org/wiki/Flocculent_spiral_galaxy
http://en.wikipedia.org/wiki/Magellanic_spiral

Referenced by pages:
AREPO
bar
Comet Galaxy
cosmic distance ladder
disk galaxy
dwarf galaxy
dwarf galaxy classification
elliptical galaxy
ESO 137-001
final parsec problem
Freeman's law
galactic bulge
galaxy
galaxy classification
galaxy formation
galaxy main sequence
galaxy merger
Galaxy Zoo
grand design spiral galaxy
Hydrogen Accretion in Local Galaxies Survey (HALOGAS)
HII region (HII)
hypergalaxy
IC 342
irregular galaxy
lenticular galaxy (S0)
Large Magellanic Cloud (LMC)
Messier 100 (M100)
Pinwheel Galaxy (M101)
Sombrero Galaxy (M104)
Messier 106 (M106)
Andromeda (M31)
Triangulum Galaxy (M33)
Whirlpool Galaxy (M51a)
M64
Messier 74 (M74)
Magellanic clouds (MC)
Milky Way
Morgan classification
NGC 253
NGC 2770
NGC 3314
Spindle Galaxy (NGC 5866)
NGC 6946
PAWS
pseudobulge
satellite plane problem
synthetic field method (SFM)
Small Magellanic Cloud (SMC)
spiral arm
spiral density wave
standard candle
stellar dynamics
Tully-Fisher relation (TFR)

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