Evidence Given By Various Teams Suggest That The Slowest Spinning Magnetar May Have Been Discovered

Astronomers who were working with NASA's Chandra Ten-ray Observatory came across some remarkable testify regarding the beingness of a dense magnetized neutron star, or better known every bit 'Magnetar'. This star was constitute at the centre of RCW 103 which is really a dense cloud of dust that has been left by a supernova lying some 10,700 lite-years away. Discovery of magnetars is always an interesting gene but what makes this different is that this star indicates signs of rotation that thousands of times slower than the usual magnetars.

Magnetar

How information technology all started?

Astronomers were first drawn towards this star in June 2022. Back then it was known equally 1E 161348-5055 or 1E 1613 for short. Antonino D'Ai led a team of researchers from Italy's Institute of Astrophysics (INAF) and they were able to option up X-ray bursts coming from this star that were similar to those of a magnetar. This particular piece of discovery was done using the NASA's Swift telescope. A magnetar is able to produce magnetic fields that are trillions of times stronger than those of the Sunday'south.According to NASA officials, "Observers had previously agreed that 1E 1613 is a neutron star, an extremely dense star created by the supernova that produced RCW 103. All the same, the regular variation in the X-ray brightness of the source, with a period of about six and a one-half hours, presented a puzzle."

This item discovery further encouraged investigation and another team led by astronomer Nanda Rea from the University of Amsterdam in the netherlands. They used NASA'southward Chandra X-ray Observatory and Nuclear Spectroscopic Telescope Assortment (NuStar). These ii technologies have the ability to search for specific bands of Ten-ray radiations in sure regions of space.
A composite image was created based on this data:

MagnetarHeaderBody

Conclusions of the various studies

Based on the obtained information which included the amount of X-rays produced and the way information technology cooled downward later on bursts, the team was able to conclude that the 1E 1613 is possibly a magnetar. Plainly, farther scrutiny must be carried out and if the data and observations are found to exist right, scientists may take discovered a 30th magnetar!

The star may have exhibited signs of being a magnetar merely in that location are still sure mysteries at mitt. D'Ai's team found that the magnetar spins, fifty-fifty though very slowly, but it still does and this is certainly non a feature that was at first assumed with the previous magnetars. NASA officials said, "The source is rotating one time every 24,000 seconds (6.67 hours), much slower than the slowest magnetars known until now, which spin around once every ten seconds. This would make it the slowest spinning neutron star always detected."

A hypothesis has been presented to answer this mystery. It is causeless that debris from the supernova, that had initially created the RCW 103 may have gotten into 1E 1613 and caused it to slow down. It is assumed that magnetars slow down with age, only if this is true, why is the 1E 1613 slowing down when it is but just two,000 years old. This fact rejects this item hypothesis. It is evident that further studies must exist washed to make any more than conclusive hypothesis regarding this star.

Till then we can hope that engineering progresses and produces better telescopes and so that nosotros tin get more information nearly such a rare kind of star.

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