The Milky Way Galaxy and the Formation of

























- Slides: 25

The Milky Way Galaxy and the Formation of Spiral Galaxies Prof. Ata Sarajedini University of Florida Department of Astronomy


The Milky Way Galaxy - Our Home Pole-On View Edge-On View


The Andromeda Galaxy - Our Nearest Large Neighbor NGC 205 M 32

• What is the significance of these satellite galaxies? They are remnants from the formation of the Milky Way’s halo! • Since the late 1970 s, theories of galaxy formation have suggested that disrupted satellite galaxies formed the Milky Way’s halo.

Satellite Galaxies of the Milky Way and Andromeda

How do dwarf galaxies get disrupted? Tidal Effects DFg DFg

The problem was that there was no concrete evidence for the buildup of spiral galaxies via the disruption and accretion of dwarf galaxies until 1994!

The “Smoking Gun” - the Sagittarius Dwarf Galaxy (Discovered in 1994) Sagittarius dwarf galaxy Velocity along the line-ofsight for stars toward the Galaxy’s Bulge stars with an average velocity of 0 km/s Blue Red


M 55 turns out to be a foreground cluster!

Observations of stars known to be a part of the Sagittarius dwarf galaxy and its tidal tails. Theoretical model of how the Sagittarius dwarf galaxy should be disrupted by the Milky Way.

• In 2003, another disrupted and digested dwarf galaxy was found… Canis Major Dwarf Galaxy

• Globular clusters are also disrupted and accreted to form the Galaxy’s halo.

• We have even detected tidal streams and tidal tails composed of stars in the halo of the Andromeda galaxy.

• The halos of the Milky Way and Andromeda do indeed show evidence of having been formed via the disruption and accretion of dwarf satellite galaxies.


Conclusion The halo of a spiral galaxy is like a bowl of spaghetti!

Today, NASA and the Space Telescope Science Institute released images of the Hubble Ultra Deep Field - the result of 11. 3 days of total exposure time with the Advanced Camera for Surveys instrument.



Satellite Galaxies of the Milky Way and Andromeda

• Similar searches for tidally disrupted dwarf galaxies around the spiral galaxy M 33 have turned up nothing significant.
