Project information
Exploring the Hot Universe and Understanding Comic Feedback
(EHU)
- Project Identification
- GX21-13491X
- Project Period
- 1/2021 - 12/2025
- Investor / Pogramme / Project type
-
Czech Science Foundation
- EXPRO
- MU Faculty or unit
- Faculty of Science
The Lambda Cold Dark Matter (Λ CDM) model has been shown to be remarkably successful in describing many aspects of our Universe, which is dominated by dark energy and dark matter. However, the physical processes associated with the evolution of the baryonic matter are complex and still poorly understood. In the course of structure formation, only a small fraction of the baryons turned into stars - most remain in a diffuse intergalactic medium (IGM). The growth of galaxies is regulated by feedback processes, such as energy and momentum input from supernovae, and jets and winds of accreting supermassive black holes. These processes, collectively called galactic feedback, can limit or even inhibit further gravitational collapse, and thus a detailed knowledge of how they work is essential for our understanding of galaxy formation and evolution. Here, I propose to take advantage of new observational opportunities to study the intimate connection between the IGM, star formation and the growth of supermassive black holes in the most massive galaxies.
Publications
Total number of publications: 52
2024
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CAvity DEtection Tool (CADET): pipeline for detection of X-ray cavities in hot galactic and cluster atmospheres
Monthly Notices of the Royal Astronomical Society, year: 2024, volume: 527, edition: 2, DOI
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Effect of Extinction on Quasar Luminosity Distances Determined from UV and X-Ray Flux Measurements
Astrophysical Journal, year: 2024, volume: 961, edition: 2, DOI
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High-spectral-resolution Observations of the Optical Filamentary Nebula Surrounding NGC 1275
Astrophysical Journal, year: 2024, volume: 962, edition: 1, DOI
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Ram-pressure stripped radio tail and two ULXs in the spiral galaxy HCG 97b
Monthly Notices of the Royal Astronomical Society, year: 2024, volume: 527, edition: 1, DOI
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The infalling elliptical galaxy M89: The chemical composition of the AGN disturbed hot atmosphere
Monthly Notices of the Royal Astronomical Society, year: 2024, DOI
2023
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A multifrequency characterization of the extragalactic hard X-ray sky: Presenting the second release of the Turin-SyCAT
Astronomy and Astrophysics, year: 2023, volume: 670, edition: February, DOI
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Accretion disks, quasars and cosmology: meandering towards understanding
Astrophysics and Space Science, year: 2023, volume: 368, edition: 2, DOI
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Broad-line region in active galactic nuclei: Dusty or dustless?
Astronomy and Astrophysics, year: 2023, volume: 680, edition: December 2023, DOI
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Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters
Astrophysical Journal, year: 2023, volume: 953, edition: 1, DOI
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Discovery of inverse-Compton X-ray emission and estimate of the volume-averaged magnetic field in a galaxy group
Monthly Notices of the Royal Astronomical Society, year: 2023, volume: 524, edition: 4, DOI