In a rare phenomenon, a one -story in a neighboring galaxy again erupted and recorded unprecedented temperatures. The explosion, which occurred in a binary star system, provided scientists with a unique opportunity to study the physical conditions of these cosmic events in a different environment than our galaxy.
According to RCO News Agency, The players occur when a white dwarf – the dense nucleus of a dead star absorbs a substance from its companion. Over time, it accumulates on the surface of the white dwarf and its temperature reaches such a terrible explosion.
Most engineers only erupt once, but some explode again after a few years to decades, and they are called recurrent players. These types of designs are very rare and few have been identified in the Milky Way. Examination of these objects in other galaxies helps to understand the impact of environmental conditions on how the players are exploded.
One of the most well -known recursive plates is the LMC2, which is located in the large Magellani cloud – near the Milky Way. It has one of the shortest recurring periods and explodes almost every four years. Researchers have long expected the crime to erupt again in year 6, and satellite observations recorded the event in a timely manner.
A group of astronomers from various institutions examined the explosion using telescopic observations. They took advantage of spectroscopy techniques in the infrared area to analyze the compounds of hot gases after the explosion. This study is the first infrared spectroscopy study of a return out of the Milky Way Galaxy.
The results of the study showed that the gases launched from this design had a temperature of about 2 million degrees Celsius, which is one of the highest temperatures recorded for this phenomenon. The researchers found that in the early stages of the explosion, the infrared light of this draft was about 5 times the sun’s brightness throughout the wave.
One of the surprising findings of this study was the presence of a very strong signal of ionized silicone atoms, while other heavy elements commonly seen in such explosions were almost absent. The discovery shows that the gases launched have reached unprecedented temperatures and that new processes are likely to be flowing in this type.
These severe conditions can be caused by the chemical properties of the large cloud. This galaxy has lower levels of heavy elements than the Milky Way, which can delay the explosion and thus it can be more severe. Also, the gases thrown from the white dwarf collided with a companion star – a red subcutter – and created a huge shock that greatly increased the temperature.
The study, published in collaboration with researchers from various institutions, was published in the journal Monthly Notices of the Royal Astronomical Society. Study data is also obtained from observations made with advanced telescopes operating under international organizations.
These findings can transform scientists’ understanding of the mechanisms of star explosions and help better predict these cosmic events in the future.
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(tagstotranslate) Blasting Blast (T) Nova (T) Chemical Signature (T) White Dwarf (T) LMC68
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