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The Stellar Initial Mass Function of Dense Stellar Systems and their Supermassive Black Holes

Public support

  • Provider

    Czech Science Foundation

  • Programme

    Standard projects

  • Call for proposals

    SGA0202600001

  • Main participants

    Univerzita Karlova / Matematicko-fyzikální fakulta

  • Contest type

    VS - Public tender

  • Contract ID

    26-21774S

Alternative language

  • Project name in Czech

    The Stellar Initial Mass Function of Dense Stellar Systems and their Supermassive Black Holes

  • Annotation in Czech

    The stellar initial mass function (IMF), i.e. the distribution of the initial masses of stars when they form, constitutes a fundamental function in astrophysics and cosmology. The IMF is the key to our knowledge of the baryonic matter content in the Universe because it is made to shine through stars. The physical conditions in the early Universe, in star-bursting galaxies, near our Sun and in the far-outer regions of our Milky Way, define what type of stars form there. In turn the formed stars affect their surroundings. We need to understand the mapping between the physical conditions and the IMF to comprehend galaxy formation and evolution. Today we understand that large concentrations of gas are dominated by short-lived massive stars, while regions with low gas density are dominated by long-lived low mass stars. The luminosity field and chemical enrichment therefore critically depend on the history of star formation and on how the IMF varies. This project will build upon our previous experience using new data to improve knowledge of the variation of the IMF.

Scientific branches

  • R&D category

    ZV - Basic research

  • OECD FORD - main branch

    10308 - Astronomy (including astrophysics,space science)

  • OECD FORD - secondary branch

  • OECD FORD - another secondary branch

  • CEP - equivalent branches <br>(according to the <a href="http://www.vyzkum.cz/storage/att/E6EF7938F0E854BAE520AC119FB22E8D/Prevodnik_oboru_Frascati.pdf">converter</a>)

    BN - Astronomy and celestial mechanics, astrophysics

Solution timeline

  • Realization period - beginning

    Jan 1, 2026

  • Realization period - end

    Dec 31, 2028

  • Project status

    Z - Beginning multi-year project

  • Latest support payment

Data delivery to CEP

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

  • Data delivery code

    CEP26-GA0-GA-R

  • Data delivery date

    Apr 27, 2026

Finance

  • Total approved costs

    12,858 thou. CZK

  • Public financial support

    12,024 thou. CZK

  • Other public sources

    834 thou. CZK

  • Non public and foreign sources

    0 thou. CZK