Indian astronomers using the NASA space telescope observed an unusual star system called SXP 138. This is the so -Called x -ray double system, where the neutron star is a very dense rest of the supernuminal explosion. Work Published on Preprint Portal Arxiv.
SXP 138 is located in a small Magellan cloud with a satellite of our galaxy. One of the characteristics of this system is the presence of a pulsar (gap source) that rotates with a period of 138 seconds and spreads strong flows of X -ray radiation.
Scientists noticed that the Pulsar rotation time has increased slightly throughout the year. This may mean that there is an area around the neutron star to prevent the purchase of the substance on the surface of the substance – it will not “push” and not attract the pulsar substance.
The authors also found a complex structure in pulsar radiation – as if they had a few bright and dull “signs önemli, which pointed in different directions. The analysis showed that radiation was drawn not only from the surface of the star, but also from the hot gas surrounding a strong gravity area.
Researchers believe that such observations will help better understand how strong the X -ray outbreaks are. In the future, they plan to continue the operation of SXP 138 and other similar systems.
Previously, scientists open The new nature of the microans in the sun.
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Source: Gazeta
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