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extensions associated with external funding. The successful applicant will work on observational studies of Active Galactic Nuclei in the High-Energy Research on Obscuration and Emission in Supermassive black
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"Accretion-ejection coupling in black-hole X-ray binaries", nr 2023/48/Q/ST9/00138, funded by the National Science Centre. The position is available for 6 months. The salary of the successful candidate will be
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Dark Matter powered stars. Those objects could be natural solutions to two of the most pressing puzzles in Astronomy today: i. the seeds of the Supermassive Black Holes powering the most distant quasars
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of galaxies and the feeding of supermassive black holes. Successful candidates will be expected to play a leading role in answering key open questions in the areas of galactic dynamics, star formation
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; HEROES : High-Energy Research on Obscuration and Emission in Supermassive black holes). The beginning of the FONDECYT fellowships is April 2025, but other dates are possible for other grants
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powered stars. Those objects could be natural solutions to two of the most pressing puzzles in Astronomy today: i. the seeds of the Supermassive Black Holes powering the most distant quasars ever observed
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electrodynamics, at the theoretical level and as applied to pulsar and black hole magnetospheres. The successful candidate will have a track record of published research in these or related areas as
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Dark Matter powered stars. Those objects could be natural solutions to two of the most pressing puzzles in Astronomy today: i. the seeds of the Supermassive Black Holes powering the most distant quasars
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further funding. This project will explore the physics of relativistic jets propagating away from black hole and neutron star X-ray binaries, specifically testing their observable properties against models
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Max-Planck-Institute for extraterrestrial Physics | Garching bei M nchen, Bayern | Germany | about 2 months ago
of the Galactic Center, and of star forming galaxies in the early Universe. We lead studies of star formation, gas content, physical properties and dynamics of galaxies, and black-hole formation and evolution