Informace o projektu
Exploring the Hot Universe and Understanding Comic Feedback
(EHU)
- Kód projektu
- GX21-13491X
- Období řešení
- 1/2021 - 12/2025
- Investor / Programový rámec / typ projektu
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Grantová agentura ČR
- EXPRO
- Fakulta / Pracoviště MU
- Přírodovědecká fakulta
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.
Publikace
Počet publikací: 71
2025
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Mapping the Filamentary Nebula of NGC 1275 with Multiwavelength SITELLE Observations
Astronomical Journal, rok: 2025, ročník: 169, vydání: 4, DOI
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MeerKAT discovery of gigahertz radio emission extending from Abell 3017 towards Abell 3016
Astronomy and Astrophysics, rok: 2025, ročník: 694, vydání: February, DOI
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MWA and VLA Observations of Diffuse Radio Lobes in M87
Astrophysical Journal, rok: 2025, ročník: 988, vydání: 1, DOI
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Optically active and optically inactive radio galaxies as sub-populations of the main galaxy sample of the SDSS
Astronomy and Astrophysics, rok: 2025, ročník: 693, vydání: January, DOI
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Red giant–jet collisions in galactic nuclei I: 3D hydrodynamical model of a few stellar orbits
Monthly Notices of the Royal Astronomical Society, rok: 2025, ročník: 540, vydání: 2, DOI
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Suzaku Observation of Merging Clusters A222 and A223
Research in Astronomy and Astrophysics, rok: 2025, ročník: 25, vydání: 6, DOI
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The bulk motion of gas in the core of the Centaurus galaxy cluster
Nature, rok: 2025, ročník: 638, vydání: 8050, DOI
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The clus model in SPEX: Projection and resonant scattering effects on the iron abundance and temperature profiles of galaxy clusters
Astronomy and Astrophysics, rok: 2025, ročník: 694, vydání: February, DOI
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The cosmological analysis of X-ray cluster surveys: VI. Inference based on analytically simulated observable diagrams
Astronomy and Astrophysics, rok: 2025, ročník: 693, vydání: January, DOI
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The warm-hot intergalactic medium in inter-cluster filaments
ASTRONOMY & ASTROPHYSICS, rok: 2025, ročník: 695, vydání: March, DOI