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Výsledek výzkumu

HD 99458: First time ever Ap-type star as a delta Scuti pulsator in a short period eclipsing binary?

CP2 stars and no unambiguously proven candidate has been reported. HD 99458We present the discovery of a unique object, a chemically peculiar Ap-type star with an orbital period shorter than 3 d. HD 99458 is there...

Astronomy (including astrophysics,space science)

  • 2019
  • Jimp
  • Odkaz
Výsledek výzkumu

HD 99458: First time ever Ap-type star as a S Scuti pulsator in a short period eclipsing binary?

stars and no unambiguously proven candidate has been reported. HD 99458 was formerlyWe present the discovery of a unique object, a chemically peculiar Ap-type star with an orbital period shorter than 3 d. HD 99458...

Astronomy (including astrophysics,space science)

  • 2019
  • Jimp
  • Odkaz
Výsledek výzkumu

HD 99458: First time ever Ap-type star as a S Scuti pulsator in a short period eclipsing binary?

stars and no unambiguously proven candidate has been reported. HD 99458 was formerlyWe present the discovery of a unique object, a chemically peculiar Ap-type star with an orbital period shorter than 3 d. HD 99458...

Astronomy (including astrophysics,space science)

  • 2019
  • Jimp
  • Odkaz
Výsledek výzkumu

Discovery of the first Ap star in an eclipsing binary system

We report the discovery of a very special object, the first star of its kind. HD 99458 appeared to be a chemically peculiar star of Ap type, showing. The spots produce rotational modulation of light variations. In addition,...

Astronomy (including astrophysics,space science)

  • 2019
  • O
Výsledek výzkumu

Three small meditation on the theme: Stars and we

1. Why we love stars so much? 2. Stars by all senses? 3. What are the stars for?...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2009
  • Jx
Výsledek výzkumu

Excitation of oscillations by a small inhomogeneity on the surface of a neutron star

inhomogeneity located on the surface of a neutron star are studied. The oscillating perturbation force in both the accretion disc rotating around the star and in the interior of a differentially rotating star is determined...

BE - Teoretická fyzika

  • 2005
  • D
Výsledek výzkumu

The nature of the light variations of chemically peculiar stars CU Vir and HD 64740

The nature of the light variations of chemically peculiar stars was studied variability of these stars, we study the light variations of the well-known magnetic chemically peculiar star CU Vir and one of the least amplitude...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2011
  • D
  • Odkaz
Výsledek výzkumu

The nature of the light variations of chemically peculiar stars

Chemically peculiar stars display periodic light and spectrum variations composition on the surface of rotating star. However, the nature of the light variations of these stars and their relationship to the spectrum variati...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008
  • D
Výsledek výzkumu

NLTE wind models of hot subdwarf stars

We calculate NLTE models of stellar winds of hot compact stars (central stars of planetary nebulae and subdwarf stars). The studied range of subdwarf parameters is selected to cover a large part of these stars. The...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2010
  • Jx
Výsledek výzkumu

A 3-D look into the atmosphere?

The atmospheres of chemically peculiar stars can be highly structured in both the horizontal and vertical dimensions. While most prevalent in the magnetic stars, these structures can also exist in non-magnetic stars. In add...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2010
  • D
  • Odkaz
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