Before the end of the black hole, many large stars blow out outer layers in powerful winds

New research indicates that very large stars with extreme monster – they more than 100 times Mass As soon as the sun – before it pushes at least 20 times more matters before it ends when they cool down to become black holes. These stars blew up a significant part of their outer layers in a very powerful dark winds during the short but intense winds of their lives, and eventually overturned the less people. One of the benefits of this extremely widespread loss is that it can calculate the strange condition of observation in the stars, such as in Tarantola Nebulla, provides new information about the source of dark evolution, the formation of a black hole, and the sources of gravity waves.

Hurricanes like hurricanes have described extremely mass damage in the most mass stars of the universe

According to A Report From Space.com, researchers used sophisticated models and observations to find out that very large stars give the winds so powerful that they act more like a hurricane than soft solar winds. Their results are very good with the observations of the WNH -type wolf rate stars in Tarantola Nebula. Improved models describe too high temperatures and hydrogen stability at the surface, which deal with previous challenges.

An important article of this study is R136A1 – the most famous star – which is 230 times more than the sun. Researchers suggested that it was either created as a single star of 200 solar people or as a binary star system where there was a joint mass of about 200 solar people in both stars. In both such cases, the star may have lost massively in the early of his life, so the results will raise the question that large -scale stars can survive for so long that such debris can be left in the big megalic cloud.

Its implications also increase to the formation of a black hole. More largely widespread winds have caused more large -scale, resulting in the manufacture of small black holes and reduces the chances of producing passionate intermediate mass black holes. This revised model also enhances matches of the gravity black hole binary with gravity wave signal.

Although these models are limited to the stars of Tarantola Nebulla, researchers have emphasized that their search is considered universal, but it is also important that the stars must be understood in different chemical environments. The results not only renounce the predictions of the Black Hole population, but also adjust our understanding of how the largest stars in the universe live – and die.