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Stars much heavier than the Sun are extremely luminous and drive strong stellar winds, blowing a large part of their matter into the galactic environment before they finally explode as  super- or hypernova. By this strong feedback, massive stars regulate the star formation and the further development of the cluster in which they were born. Massive stars generate most of the ultraviolet radiation of galaxies -- the whole Universe was re-ionized by the first (super)massive stars -- and power their infrared luminosities. Massive stars are bright signposts that help to determine the age, scale, shape, and content of the Universe. Quantitative knowledge of the action of massive stars is prerequisite to comprehend the Universe we see.
 
 

                                                                                  LO's Main  Research  Iterests
 
SXP1062 and NGC602

Long period pulsar SXP 1062 and star cluster NGC602 in the Small Megenllanic Cloud.

X-ray: NASA/CXC/Univ.Potsdam/L.Oskinova et al & ESA/XMM-Newton;

Optical: AURA/NOAO/CTIO/Univ.Potsdam/L.Oskinova et al

  • X-ray emission from massive stars

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  • Massive stars in the Milky Way center

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  • Radiative transfer in stochastic medium

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  • High-Mass X-ray binaries

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  • Magnetism in massive stars

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  • Massive stars and star formation at low metallictiy