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department exoplanet news

European Southern Observatory – Queen of Astronomy

2024-02-282024-02-28 admin

On 22-24 February 2024, the Brno Observatory and Planetarium together with the ESON-Czech group promoting the European Southern Observatory organised a series of lectures and

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hotstars news

A seven-Earth-radius helium-burning star inside a 20.5-min detached binary

2024-02-122024-03-20 admin

Professor Xiaofeng Wang’s team at Tsinghua University and their collaborators (including Péter Németh from the Stellar Department of the Astronomical Institute in Ondřejov) have made

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exoplanet news

The evaporation of planetary atmosphere

2024-01-162024-02-12 admin

In the field of exoplanet research, astronomers have already moved on from simply discovering new objects to characterising them. Not only are the parameters of

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hotstars news

On the stability and pulsation in models of B[e] star MWC 137

2024-01-122024-02-12 admin

Giant stars of spectral type B with emission lines in their spectrum have been the long-term research focus of Michaela Kraus of ASU’s Stellar Department.

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department highenergy news

14th Annual International Conference on X-ray Optics in Astronomy

2023-12-052024-02-12 admin

An international meeting of experts in X-ray astronomy – AXRO 2023 – will take place in Prague from 4 to 8 December, bringing together the

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News

  • Stellar obliquities of eight close-in gas giant exoplanets
  • HD 144812 – A transition-phase massive star in a binary system
  • Our Erasmus+ project has been nominated
  • Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1
  • Chat with an astronomer 2025
  • Horizontal flows in the atmospheres of chemically peculiar stars
  • Spectroscopy of comet C/2023 A3 (Tsuchinshan-ATLAS)
  • Exceptionally Large Transit Timing Variations Induced by Two Resonant Warm Gas Giants in a Three-planet System
  • PLATOSpec – the new instrument at ESO’s La Silla Observatory is now ready for exoplanet research
  • TOI-2458 b: A mini-Neptune consistent with in situ hot Jupiter formation

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