Hot Stars and Stellar Winds
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What we do
In particular, we provide theoretical background and computational tools to investigate different populations of massive stars, in the Milky Way, the Magellanic Clouds, and low-metallicity Local Group galaxies. These investigations are performed using various observational surveys in the optical and partly UV, such as FLAMES I and II, ULLYSES, XshootU and IACOB. These international collaborations feature members from (among others) the Universities of Leuven (Belgium), Amsterdam (Netherlands), La Laguna (Tenerife, Spain) and Madrid (Spain).
© Hubble Archive / Judy Smith
People
| Name | Tel | Room | Position | |
|---|---|---|---|---|
| Puls, Joachim | uh101aw@usm.uni-muenchen.de | +49 89 2180-6022 | 118 | University Observatory Munich |
| Hoffmann, Tadziu | hoffmann@usm.lmu.de | 089-2180-6024 | 118 | Scientific Staff |