Keyword: Astronomy

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Radio signal reveals supernova origin

17.05.2023

In the latest issue of the journal Nature, an international team including astronomers from University of Turku reveal the origin of a thermonuclear supernova explosion. Strong emission lines of helium and the first detection of such a supernova in radio waves show that the exploding white dwarf star had a helium-rich companion.

Astrophysicists discover a puzzlingly perfect spherical explosion in space

16.02.2023

When neutron stars collide, they produce a violent explosion. Data from the only well observed collision show that the explosion was perfectly spherical, completely contrary to expectations. How this is possible remains a mystery, but the discovery may provide a new key to fundamental physics and to measuring the age of the Universe. The discovery was made by an international collaboration led by astrophysicists from the University of Copenhagen and including researchers from the University of Turku. The research has just been published in the journal Nature.

Astronomers from the University of Turku to scan the sky in search of optical signals from gravitational waves

21.07.2022

The department of Physics and Astronomy at the University of Turku is a partner in the international Gravitational-wave Optical Transient Observer (GOTO) project, which will play a key role in shepherding in a new era of gravitational wave science. The GOTO observatory is made up of two identical telescope arrays on opposite sides of the planet that will track down sources of gravitational waves resulting from violent cosmic events that create ripples in the fabric of space-time itself.

Observations of the centres of galaxies reveal the hidden destruction of stars by lurking supermassive black holes (Dissertation defence Nov 4 2021, MSc Thomas Reynolds, astronomy)

We know that in the centres of the majority of galaxies lies a supermassive black hole. New observations of certain galaxies reveal that these black holes may be consuming stars at a higher rate than previously known. The energy produced by the destruction of the star can be revealed in the infrared, as heat from cosmic dust warmed by the explosion.
 

Polarization of Light Helps to Better Understand Emission Sources in the Vicinity of Stellar-Mass Black Holes (Dissertation Defence, MSc Ilia Kosenkov, 8 Oct 2021, Astronomy)

Stellar-mass black holes that are part of binary systems sometimes show variable polarization of optical emission. The degree, angle and variability pattern of polarization is characteristic of the physical processes occurring in the vicinity of a black hole. By studying black holes astronomers learn how matter and energy behave under extreme conditions.