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2 593 (0,084s) •

Project

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

. One of the star formation modes is the so called triggered star formation in which one episode of star formation leads to the creation of a dense and thin expanding. In other words, star

BN - Astronomie a nebeská mechanika, astrofyzika

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

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

The formation of star clusters with masses higher than 10^5 Solar masses clouds is converted to stars, i.e. what is the star formation efficiency in massive star clusters. Currently, there is a di...

Astronomy (including astrophysics,space science)

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

Asymptotic normalization coeficients in nuclear astrophysic. (ME 643)

Main goal of project is to acquire new knowledge about evolution and forming of stellar enviroment,aboutenergetical evolution of stars,about processes leading to formation of stars and processes leading to its extinction......

BG - Jaderná, atomová a molekulová fyzika, urychlovače

  • 2003 - 2005
    • •
  • 1 756 tis. Kč
    • •
  • 1 756 tis. Kč
    • •
  • MŠMT
Project

Black holes and their environment (LD12065)

into account gravitational interaction of a supermassive black hole (SMBH), stars and gaseous structures as well as the hydrodynamical interaction of stars and gas. We will assume formation of stars via fragmentat...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2012 - 2014
    • •
  • 1 189 tis. Kč
    • •
  • 1 189 tis. Kč
    • •
  • MŠMT
Project

Multi-Generation Star Clusters (GA15-06012S)

of multiple generations of stars in globular clusters. We will explore the cluster mass UV photons to cool down to low temperatures and become seeds of secondary star formation. We shall compare the emission line profiles ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2015 - 2017
    • •
  • 5 406 tis. Kč
    • •
  • 5 406 tis. Kč
    • •
  • GA ČR
Project

B[e] supergiants where is their place within the evolution of massive stars? (KJB300030701)

Several phases during the evolution of massive stars are still not or not well symmetric winds and the formation of their (neutral) disks. The goal of this project is to find their place in the evolution of massive stars. W...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2007 - 2009
    • •
  • 1 624 tis. Kč
    • •
  • 1 624 tis. Kč
    • •
  • AV ČR
Project

Unveiling the population of close-in exoplanets and brown dwarf companions to stars (GN23-06384O)

stars (F-type and A-type stars) remain relatively unexplored because to understanding the impact of stellar properties on the formation and evolution of substellar BDs around intermediate mass stars. (2) By using ...

Astronomy (including astrophysics,space science)

  • 2023 - 2026
    • •
  • 4 655 tis. Kč
    • •
  • 4 655 tis. Kč
    • •
  • GA ČR
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

BN - Astronomie a nebeská mechanika, astrofyzika

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

Astrophysics and dynamics of the solar atmosphere, bodies and matter of the solar system, non-stationary stars and galaxies (KSK1003601)

Formation of stars and dynamics of galaxies. Eruptive processes in cosmic plasma. Interacting binary stars, an analysis of their geometry and physics of the star surrouding mass. Spectroscopy and interferometry of ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1996 - 2000
    • •
  • 55 274 tis. Kč
    • •
  • 37 691 tis. Kč
    • •
  • AV ČR
Project

Aperiodic short-term phenomena in Be star spectra as potential magnetic field (IAA3003403)

understanding not only of Be star disk formation, but of hot stars in general.Disks of many Be stars are known to form through outbursts. In some stars, non pulsation variability, Be star absorpt...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2004 - 2005
    • •
  • 511 tis. Kč
    • •
  • 141 tis. Kč
    • •
  • AV ČR
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