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2 342 (0,097s)

Project

Mass loss in hot massive stars (GA13-10589S)

of the amount of mass lost in individual evolutionary stages. However, the mass-loss rate project will overcome these limitations and will provide reliable mass-loss rate predictions for a broad range of ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2013 - 2017
  • 8 796 tis. Kč
  • 8 796 tis. Kč
  • GA ČR
Project

Mass-loss in evolved massive stars (GA18-05665S)

of the cosmic dawn. The amount of mass lost per unit of time, that is, the mass-loss rate mass-loss rate predictions in evolved massive stars. These predictions of limiting cases will shed light on episod...

Astronomy (including astrophysics,space science)

  • 2018 - 2020
  • 7 630 tis. Kč
  • 6 750 tis. Kč
  • GA ČR
Project

Mass-loss rate predictions for hot stars (GA205/08/0003)

Massive hot stars constitute an important part of our Galaxy and many other galaxies. Consequently, a detailed knowledge of their evolution and of their influence on the circumstellar environment is necessary for our understanding of the structure an...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2012
  • 4 876 tis. Kč
  • 4 876 tis. Kč
  • GA ČR
Project

Hot star winds solving uncertainties of mass loss near the Eddington limit (GA25-15910S)

. To understand these processes, a detailed knowledge of the amount of mass lost per unit of time (mass-loss rate) is needed. However, such information is missing for luminous-of-the-art codes. We will provide precise m...

Astronomy (including astrophysics,space science)

  • 2025 - 2027
  • 12 728 tis. Kč
  • 12 728 tis. Kč
  • GA ČR
Project

Tracing the mass-loss history in evolved massive stars (7AMB14AR017)

In this collaboration project we will study the mass-loss history in evolved the strongly enhanced mass-loss in these short-lived phases together with proper estimatesof the mass-loss rates in the...

BN - Astronomie a nebeská mechanika, astrofyzika

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

Revealing the pulsation-induced mass loss of blue supergiants and its interplay with the interstellar medium (GA25-17532S)

their pulsation properties and the power of pulsations to induce mass loss. For this, we...

Astronomy (including astrophysics,space science)

  • 2025 - 2027
  • 17 018 tis. Kč
  • 17 018 tis. Kč
  • GA ČR
Project

Unveiling the mass-loss history of evolved massive stars (GA14-21373S)

. The project thus addresses the important issue of the mass-loss history in these twoThe post-main sequence evolution of massive stars contains several short-lived phases such as the luminous blue variable and the B[e] supergiant p...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2014 - 2016
  • 4 997 tis. Kč
  • 4 997 tis. Kč
  • GA ČR
Project

Circumstellar envelopes of hot stars (GA205/04/1267)

the mass-loss rates. Calculated spectra will be compared with the observed ones both exact wind parameters (mass-loss rates and terminal velocites) will be the output......

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2004 - 2006
  • 2 722 tis. Kč
  • 2 722 tis. Kč
  • GA ČR
Project

Binary interaction on the red giant branch Hot subdwarfs as a test case. (GA22-34467S)

The impact of binarity on the evolution of low-mass stars is an important and yet poorly understood domain of stellar astrophysics, yet it results in a diverse physics in low- to intermediate-mass stars, specifically by establishing...

Astronomy (including astrophysics,space science)

  • 2022 - 2024
  • 8 324 tis. Kč
  • 8 324 tis. Kč
  • GA ČR
Project

Shed more light on magnetic stars (7AMB14AT015)

We aim toward new insights of the magnetic chemically peculiar (mCP) stars of the upper main sequence. This star group is an excellent astrophysical laboratory for testing processes like diffusion, accretion, and mass loss. The foun...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2014 - 2015
  • 132 tis. Kč
  • 132 tis. Kč
  • MŠMT
  • 1 - 10 out of 2 342