Astronomers discovered teleioos, perfect symmetry with a supernova residue

A supernova residue (SNR) with extraordinary circular symmetry has been seen by an international team of researchers. Supernova residue (SNR) is the remains of a supernova explosion, which is seen as spread, expansion structures. The observation suggests that the SNRS expands the port to the port extended by the supernova explosion. They also contain other intersteler materials that are washed away by the passage of Shockwave from the explosive star. Rather unusual SNR is named “Teleos”, which is the Greek word right. Newfound SNR was officially nominated as the G305.4–2.2, which was identified in the Radio-Kantinum images of the Australian square km-kilometer array of the universe (EMU) (EMU).

Abnormal structure and property

As Research paper Describing the “teleos”, it stands for its unusual symmetrical structure. SNRs are usually unrelated due to uneven distribution of intersteller medium (ISM), in which they expand. LSNR J0624–6948, SN1987A, or MC SNR J0509–6731 shows some remains similar morphology

According to the paper, G305.4–2.2 or “teleos” is located at a distance of 7,170 or 25,100 light years to suit the diameter of 45.6 or 156.5 light years respectively. Study Some extended radio emissions were found inside the south -east edge of the shell of Telios. This suggests that at least some parts of the region may be affected by the interaction of teleos with local intersteller medium (ISM) structures. A steep spectral index of -0.6 suggests that the residue is either relatively young or too old and displays a lower surface shine. These features make teleos a compelling goal for intensive examination.

Possible origin and future research

The authors of the study proposes that teleoses were likely to be from a type of IA Supernova, possibly built under the Galactic aircraft of Milky Way. However, no direct evidence currently confirms this hypothesis. To highlight more about the original and development of teleos, researchers recommend future high-resolution, multi-discharge comments.

These can reveal its expansion velocity and provide a clear picture of its age and composition. Such efforts will not only enhance the understanding of this unique remains, but also provide wide insight into the variety and behavior of supernova explosions in our galaxy.