Contact

Rix, Hans-Walter
Hans-Walter Rix
Managing director

Phone: +49 6221 528-210
Room: 216 D
Bailer-Jones, Coryn
Coryn Bailer-Jones
Phone: +49 6221 528-224
Room: C 5
Bergemann, Maria
Maria Bergemann
Independent Research Group Leader

Phone: +49 6221 528-401
Room: 330

Milky Way and Local Group

The observed stars from the Gaia-ESO survey superimposed on a model Galaxy. Zoom Image
The observed stars from the Gaia-ESO survey superimposed on a model Galaxy.

The Milky Way with its cohort of small satellite galaxies are almost the only galaxies that can be studied star-by-star and that can be mapped in 3D: an ideal testbed for understanding galaxy assembly. Along with the Milky Way's big neighbour, the Andromeda galaxy, and a few smaller galaxies they form the 'Local Group'.

The unique detail in which we can study the Local Group makes those most nearby galaxies model organism for understanding how galaxies were assembled:

  • we can see where the stars that formed early live and on what orbits they move
  • we can see how many shreds from earlier mergers of galactic sub-units are still left over
  • only in the Milky Way do we have a chance to see the faintest galaxies in the Universe
  • only there can we which fraction of the gravitational mass is flat (e.g. a stellar disk) and or spheroidal (a dark matter halo).

Recent and ongoing systematic mappings of the night sky (SDSS, Pan-STARRS) have 100-folded the observational information in the last years, and have e.g. unveiled the presence of numerous, almost completely dark dwarf galaxies in their outer regions. Stellar streams, produced by their destructive journey near the Milky Way or Andromeda, are now seen and interpreted as the signposts of the ongoing formation history of these two massive spiral galaxies. The Gaia mission is measuring the phase-space coordinates (positions and velocities) of over a billion stars, and spectrophotometry of hundreds of millions of sources, and is bringing about a revolution in our understanding of the formation of our galaxy and the nature of its stellar and dark matter content.

Associated Research Groups

MPIA's Milky Way group uses a number of powerful tools (including imaging and spectroscopic surveys, dynamical models, and numerical simulations) that, when combined produce a comprehensive and detailed picture of our galaxy today.

Milky Way Group

MPIA's Milky Way group uses a number of powerful tools (including imaging and spectroscopic surveys, dynamical models, and numerical simulations) that, when combined produce a comprehensive and detailed picture of our galaxy today. [more]
The MPIA hosts one of two Gaia teams in Heidelberg. This team plays a leading role in CU8 "Astrophysical Parameters", by developing algorithms to classify and interpret the Gaia data. 

Gaia Group

The MPIA hosts one of two Gaia teams in Heidelberg. This team plays a leading role in CU8 "Astrophysical Parameters", by developing algorithms to classify and interpret the Gaia data.  [more]
This research group applies the methods of spectroscopy to study stars—the fundamental units of the Universe. They observe the Sun and other stars on large telescopes and use the measured spectra to study the structure and properties of stellar ‘atmospheres.'

Stellar Spectroscopy and Populations Group

This research group applies the methods of spectroscopy to study stars—the fundamental units of the Universe. They observe the Sun and other stars on large telescopes and use the measured spectra to study the structure and properties of stellar ‘atmospheres.' [more]
 
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