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department hotstars news

The “LELOIR” prize for Dr. Michaela Kraus

2022-05-162022-05-16 admin

Dr. Michaela Kraus from the Stellar Physics Department was awarded by the “LELOIR” prize 2021 from the Ministerio de Ciencia, Technologia e Innovacion of Argentina,

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hotstars news

Stellar wind research contributed to a better understanding of massive stars

2022-03-152022-04-12 admin

The Czech Science Foundation (GA CR) announced the final evaluation of project no. 18-05665S ‘Mass loss in the late evolution stages of massive stars’ which

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hotstars news

Revisiting the evolved hypergiants in the Magellanic Clouds

2022-03-102022-04-12 admin

A team of astronomers led by Michalis Kourniotis (Department of Galaxies and Planetary Systems, AI) and Michaela Kraus (Stellar Department, AI) focused on refining data

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hotstars news

HR 6819 is a binary system with no black hole

2022-03-022022-03-02 admin

In 2020 a team led by European Southern Observatory (ESO) astronomers reported the closest black hole to Earth, located just 1000 light-years away in the

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hotstars news

Bouncing against the Yellow Void – exploring the outbursts of ρ Cas from visual observations

2022-01-192022-03-10 admin

Michaela Kraus from the ASU Stellar department together with Grigoris Maravelias from Greece studied the episodes of dimming connected with a mass loos of 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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