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9 506 (0,158s) •

Project

Accurate physical properties of hot stars based on binary and multiple star studies (GAP209/10/0715)

The goal of the project is to contribute both methodologically and via new observations and their analyses to the improvement of basic physical properties of stars in binary and multiple systems. Only accumulation of a suff...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2010 - 2014
    • •
  • 5 360 tis. Kč
    • •
  • 5 360 tis. Kč
    • •
  • GA ČR
Project

Integration of prof. Guillermo Contreras in activity of Centre for Physics of Ultra-relativistic Heavy Ion Collisions at FNSPE CTU (LK11209)

Implementation of direct cooperation between FNSPE CTU and CINVESTAV Merida, Mexico, Study of production of multi-strange particles in ALICE experiment, Study of properties of the deconfined nuclear matter in ALICE and STAR experime...

BF - Elementární částice a fyzika vysokých energií

  • 2012 - 2016
    • •
  • 14 914 tis. Kč
    • •
  • 14 914 tis. Kč
    • •
  • MŠMT
Project

Collaboration on a complex study of hot stars (ME 402)

Study of the short-term variations in hot stars to determine their physical properties using models of oscillations and corotating structures Study of the nature of long-term variations of the Be envelopes in an effort to t...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2000 - 2002
    • •
  • 823 tis. Kč
    • •
  • 527 tis. Kč
    • •
  • MŠMT
Project

Spectroscopy and Numerical Modeling of Stellar Atmospheres (IAA300030908)

. In particular, compact stars such as white dwarfs cover ranges of physical parameters, high the physics of stars. The project will confront multiwavelength spectroscopic data to sets beyond the iron group. The ob...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2009 - 2011
    • •
  • 2 375 tis. Kč
    • •
  • 2 375 tis. Kč
    • •
  • AV ČR
Project

Study of new properties of nuclear matter in the international experiment STAR (LTT18002)

of the STAR detectors and RHIC performance. RHIC is currently the only fully dedicated accelerator of heavy-ions. In upcoming years, the STAR physics programme will focus collisions in the international experiment STAR...

Nuclear physics

  • 2018 - 2022
    • •
  • 21 216 tis. Kč
    • •
  • 21 216 tis. Kč
    • •
  • MŠMT
Project

Star formation triggered by expanding shells (GAP209/12/1795)

including properties of the resulting stellar population and identify physical processesUnderstanding how stars are formed is an important problem of modern. One of the star formation modes is the so called trigge...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2016
    • •
  • 9 971 tis. Kč
    • •
  • 9 971 tis. Kč
    • •
  • GA ČR
Project

Neutron stars and pulsars (LTC18058)

Main goals of the projects are estabilishment of scientific group that will work in the field of neutron stars on international level and will participate in the COST Action CA16214 The multi-messenger physics and astrophysics of n...

Astronomy (including astrophysics,space science)

  • 2018 - 2021
    • •
  • 3 843 tis. Kč
    • •
  • 3 843 tis. Kč
    • •
  • MŠMT
Project

Magnetic stars - laboratories of stellar physics (MEB060807)

physical processes that make these magnetic stars important laboratories of stellar physics. Collaboration between both participants of the project will consistThe aim of the project is the common complex research of the p...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2009
    • •
  • 95 tis. Kč
    • •
  • 95 tis. Kč
    • •
  • MŠMT
Project

Physics of Sun, stars, and stellar systems (GD205/08/H005)

exploits results of related sciences, especially physics. Demands on young scholars,who of astrophysical plasma, which exists in Sun, stars, stellar systems and their surroundings. Plasma behaviour and properties then dete...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2011
    • •
  • 10 687 tis. Kč
    • •
  • 10 687 tis. Kč
    • •
  • GA ČR
Project

Improving physics of hot stars via observations of suitably selected binaries (GA205/06/0304)

Using suitably selected binaries containing O and B stars, we shall: (1) study the effects of rapid rotation on the stellar radiative properties via observations of eclipsing andnon-eclipsing binaries, (2) test the stellar internal ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2006 - 2008
    • •
  • 2 430 tis. Kč
    • •
  • 2 430 tis. Kč
    • •
  • GA ČR
  • 1 - 10 out of 9 506