Splinter Meeting Populations

Stellar Populations in and around the Milky Way

Time: Tuesday September 19, 14:00-16:30 and Wednesday September 20, 17:00-19:00

Room: HS5

Convenors: S. Kamann (Liverpool), E. K. Grebel (Heidelberg), M. Hilker (Garching), E. Starkenburg (Potsdam), S. Dreizler (Göttingen), T.-O. Husser (Göttingen)

Our view of our cosmic neighbourhood is getting more and more detailed. With the Hubble Space Telescope, it became possible to resolve many members of the Local Group into individual stars, a legacy that will soon be continued by its successor, the James Webb Space Telescope. In the meantime, our Galaxy is being surveyed in unprecedented detail by the Gaia satellite and wide-field imaging surveys are continuing to discover its faintest companion galaxies. In the not too distant future, the E-ELT will push the study of resolved stellar populations towards local volume galaxies.

Spectroscopic follow-up is indispensable for the interpretation of the photometric and astrometric data, therefore the advent of powerful spectrographs marked a cornerstone for the study of resolved stellar populations. On small scales, integral-field spectrographs such as KMOS or MUSE allow us to target individual stars even in crowded stellar fields nowadays. On larger scales, the next generation of multi-object spectrographs (including 4MOST or the proposed MOSAIC instrument) will soon revolutionise our capabilities for wide-field spectroscopic surveys.

The purpose of this splinter is to bring together the German community working on optical/NIR spectroscopy of resolved stellar populations. We plan to discuss the current status of the field, identify open questions, and exchange about new ideas with current and future observing facilities. The topics we aim to cover include (but are not exclusive to)

  • The spectroscopic view of Gaia on the Milky Way
  • The stellar populations in star clusters and their dynamics
  • The smallest satellites in our Local Group
  • Star formation histories of nearby galaxies
  • Wide fields vs. crowded fields – combining multi-object and integral-field spectroscopy

We plan to have a healthy mix of contributed and invited talks. Graduate students are especially encouraged to apply.

Program

Related contributions *)

PresentationTitleType PDF
ArentsenUncovering metal-poor stars in the Galactic bulge with the Pristine surveyTalk PDF
El-YoussoufiMorphology and Spatial distribution of Stellar Populations in the Magellanic Clouds from the VMC surveyTalk PDF
GiesersBinary stars in Galactic globular clustersTalk PDF
GuiglionThe AMBRE Project: r-process element abundances in the Milky Way thin and thick discsTalk PDF
GöttgensSearch for emission line objects in Galactic globular clustersTalk PDF
HeberHypervelocity starsTalk PDF
HämmerichMUSE spectroscopy of Horizontal Branch stars in omega Cen and NGC 6752Talk PDF
Jong4MOST - The facility to spectrally explore Stellar Populations in and around the Milky WayTalk PDF
JordanThe Gaia Mission - Overview, First Results, and future prospectsTalk PDF
KochStellar populations in the bulge - from no-resolution to high-resolutionTalk PDF
LatourSpectroscopic insights on the extreme horizontal branch population of omega CentauriTalk PDF
MolinskiMultiple stellar populations in globular clustersPoster PDF
RamachandranStellar population of the superbubble N 206 in the LMCTalk PDF
ShenarThe Wolf-Rayet population in the Magellanic Clouds and implications on star formationTalk PDF

*) submitted abstracts, acceptance pending.