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455 (0,239s) •

Project

Star formation efficiency in massive star clusters (GA19-15008S)

clouds is converted to stars, i.e. what is the star formation efficiency in massive star clusters. Currently, there is a discrepancy between theoretical models predicting that the star formation efficienc...

Astronomy (including astrophysics,space science)

  • 2019 - 2022
    • •
  • 6 233 tis. Kč
    • •
  • 5 990 tis. Kč
    • •
  • GA ČR
Project

F. Magellanes support of ground- and space-based study of stars and stellar systems in the Galaxy and Magellanic clouds (LG15010)

The project F. Magellanes supports the study of stars using the photometric observations with Danish 1.54 m teleskope at the La Silla Observatory (ESO) in Chile will be used for the study of selected stars and peculiar objects in th...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2015 - 2017
    • •
  • 3 143 tis. Kč
    • •
  • 3 143 tis. Kč
    • •
  • MŠMT
Project

Magellanic Clouds - evolution, interaction history and formation of large-scale structures (GPP209/11/P699)

Clouds (LMC, SMC), and to reflect the today's challenges regarding the interactions of the Clouds within the Local Group of Galaxies. Improvements of his own self-consistentN-body/gas dynamics model of the Magellanic Clouds

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2011 - 2013
    • •
  • 1 374 tis. Kč
    • •
  • 1 374 tis. Kč
    • •
  • GA ČR
Project

Study of properties of asteroids and stellar systems with photometric observations with the Danish 1.54-m telescope at the European Southern Observatory (LG12001)

in the Magellanic Clouds, derivation of their distances. Study of rotational periods of chemically peculiar stars in the Magellanic Clouds.......

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2014
    • •
  • 13 695 tis. Kč
    • •
  • 3 670 tis. Kč
    • •
  • MŠMT
Project

Numerical simulations of environmental effects in galaxy clusters (GP205/08/P556)

canbe swept out and frequently observed HI-deficient galaxies with a quenched star galaxy orbits on the stripping efficiency and on the process of star formation which isconnected to the presence of cold molecular clouds i...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2010
    • •
  • 420 tis. Kč
    • •
  • 420 tis. Kč
    • •
  • GA ČR
Project

Applications of astronomical all-sky cameras and their data reduction and analysis (7AMB14AR005)

The goal of this project is to operate and collect data from automatic all-sky cameras in co-operation with scientific collaborators from Argentina. The cameras were developed by the Czech partner and are located in three different areas in Argentina...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2014 - 2015
    • •
  • 320 tis. Kč
    • •
  • 320 tis. Kč
    • •
  • MŠMT
Project

Formation of carbon molecules and dust in astrophysical environments (LUC24023)

) symbiotic binaries and (ii) star-forming regions. The main questions we want to answer are the following: 1) Can the surrounding dust shells around symbiotic stars persist and expand survey of large-scale dust nebulae around symb...

Other natural sciences

  • 2024 - 2026
    • •
  • 7 406 tis. Kč
    • •
  • 7 406 tis. Kč
    • •
  • MŠMT
Project

Stellar winds of first stars in the Universe (GA205/07/0031)

Chemical composition of first stars in the Universe was given by the primordial nucleosynthesis: first stars were composed basically only from hydrogen and helium. Numerical simulations of their formation show that first stars

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2007 - 2009
    • •
  • 1 681 tis. Kč
    • •
  • 1 681 tis. Kč
    • •
  • GA ČR
Project

Investigations of curious variable stars (LH14300)

The aim of project is to investigate of curious variable stars as contact and near-contact binaries, binaries with variable components, RR Lyrae type stars with Blazhko event or chemical peculiar stars. Output of the projec...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2014 - 2015
    • •
  • 798 tis. Kč
    • •
  • 798 tis. Kč
    • •
  • MŠMT
Project

Spectral energy distribution of hot stars and its variability (IAA301630901)

stars used to be explained by the presence of spots with uneven energy distribution on the surface of rotating stars. A typical example are chemically peculiar stars, but a similar type of the light variability is expected...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2009 - 2011
    • •
  • 2 443 tis. Kč
    • •
  • 2 443 tis. Kč
    • •
  • AV ČR
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