Data from the HESS observatory in Namibia has led to the discovery of the most energetic gamma rays ever detected from a dead star known as Tepar.
According to Tekna technology and technology news service, the discovered gamma rays reach 20 tera electron volts or about 10 trillion times the energy of visible light. Pulsars, which are the remnants of exploded stars in a nova cloud, have a giant magnetic field and are usually small in diameter. Dead stars and composed of neutrons have a very high density, so that a very small volume of them, the size of a teaspoon, can have a mass of 5 billion tons.
These star fevers usually emit columns of electromagnetic radiation as they rotate. If their rotation is in the direction of the solar system, their radiation flashes will be visible in the solar system at regular intervals. According to scientists, the source of the radiation is probably the high-speed electrons in the plasma of the stellar fever magnetic field, which are accelerating and release their absorbed energy in the form of radiation when they leave the magnetic field. Currently, scientists have discovered another radiation sense with the observations of the observatory, which is in the range of gamma rays and has about tens of tera electron volts of energy. To create such energy, electrons must move out of the magnetic field and at a great distance. Of course, the rotation pattern of radiation will still be preserved.
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