Very large stars blow the outer layers in the powerful winds before the fall of the black hole.

New research indicates that the most demonic giant stars – which are more than 100 times On a large scale As the sun – at least 20 times more cases they think to do this than before they are cold because they cool to become a black hole. These stars blow an important part of their external layers in a brief but acute curriculum of their life into quite powerful stellar winds, which finally leave the low public behind. An advantage of this extreme mass loss is that it can be responsible for the strangeness seen in those stars in Tarantula Nebula, which provides new information on sources of stellar development, black hole formation and gravity waves.

Stormy winds like storm explain extreme mass loss in the largest stars of the universe

As Report From Space.com, researchers used sophisticated models and comments to find out that very large stars give the winds so powerful that they function more like a storm than soft solar winds. Their results are very well agreed with the comments of the WNH-type Wolf-Rit stars in Tarantula Nebula, which are expected and more compact by the standard model. Better models explain very high temperatures on the surface and stability of hydrogen, which address the previous challenges.

A major theme in this study is R136A1 – the largest known star – with mass up to 230 times the sun. Researchers suggested that it is formed either as a single star of about 200 solar mass or as a binary star system, where both stars had a combined mass of about 200 solar mass. In both such cases, the star would have lost large amounts of mass in his life, so the conclusion would question how it is that large -scale stars can live longer to leave such debris in large magelli clouds.

Implications also expand to the formation of black holes. More large-scale stellar winds destroy more mass, resulting in the production of small black holes and decreasing the chances of creating elusive intermediate-mas black holes. This amendment also enhances models’ matches, which is a garautavashan wave indication observed of a Geloeing Black Hole Binary.

Although models are limited to stars in Tarantula Nebula, researchers emphasize that their findings are also important to understand stars in various chemical environments, to be considered universal. The results not only reopen the predictions of the black hole population, but can also adjust our understanding of how the largest stars live in the universe – and die.