Teleios astronomers, which are supernova residue with perfect correspondence

Supernova (SNR) residue was discovered with an exceptional circular consistency by an international team of researchers. Supernova (SNRS) residue is the Supernova explosion, which is seen as widespread and expanded structures. Notes indicate that the SNRS port removed the expanding materials from the Supernova explosion. It also contains other substances among the stars that were swept by the shock wave from the explosive star. This SNR is somewhat unusual “Teleios”, the Greek term for perfection. The newly discovered SNR, officially appointed as G305.4-2.2, was identified in the Austain Array Pathfinder (ASKAP) radio.

Unusual structure and characteristics

According to Search paper He describes “Teleios”, and it stands out because of its unusual the same structure. SNRS is generally non -asymmetric due to the unequal distribution of the medium among the stars (ISM) in which it expands. A few residue like LSNR J0624-6948, SN1987A or MC SNR J0509-6731 Similar Morphology Gallery

According to the paper, the G305.4-2.2 or “Teleios” is located 7170 or 25100 light years, corresponding to a diameter of 45.6 or 156.5 light years, respectively. the Ticket Some radio emissions extended inside the southeastern edge of the Teleios shell. This indicates that at least some parts of this region may be affected by the interaction of Teleios with medium structures (ISM) among local stars. A very slope spectrum index notes to -0.6 that the remains of either relatively young or very old and the brightness of a low surface appears. These features make Teleios a convincing goal for deeper achievement.

Possible origins and research in the future

The authors of the study suggest that Teleios is likely to have originated from the type IA Supernova, and may be formed under the galaxy plane in the Milky Way. However, there is no direct evidence currently confirming this hypothesis. To reveal more about Teleios’s origin and development, researchers recommend high -resolution notes in the future.

This expansion speed can reveal and provide a clearer image about its life and its composition. Such efforts will not only enhance the understanding of these unique remains, but also provide wider visions of the diversity and behavior of the explosions of the faults in our galaxy.