Something Unexpected Is Spewing Stars Into the Milky Way

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New research from A team of Harvard Center for Astro Physics suggests that the greater Magelonic Cloud, a dwarf galaxy neighbor Milky WayA few thousand times mass by hosting an gravitational structure Sunshine: A potential supermasive black hole.

The most recognized theory of the galactic evolution contains that supermasive black holes are found in the largest galaxies like Milkyo only. Until now, there was no reason to imagine that a small cluster like the big Magelic Cloud could host a host. When X-ray telescopes or observations are trained in a small cluster like large Magelic Cloud, they did not find any signature related to the Blackhole activity.

But then the hypervelository stars came. For about 20 years, astronomers spotted fast traveler stars with adequate acceleration to get out of their own galaxy. When a traditional tidal stars moves about 100 km per second, a hypervolosis star travels 10 times faster. Experts believe that these national stars appear to be “catalpulated” by a supermasive gravitational structure under the hill system – which a binary star system communicates with a black hole, captured by a star black hole and moves away from it.

The Milky Way itself is in the hypervelository stars that probably originated here. Studies indicate that they were accelerated by the supermasive black hole, bow a*at the center of the galaxy. However, at least 21 hypervolti stars are consistent with a supermasive black hole detected but they may not be associated with the internal activity of Milkyo. In the simulations of the team, it is commendable that these stars are derived from the big Magelic cloud instead of.

For the team led by Gion Jesse Han, this is one of the first major pieces of evidence for the presence of a supermasive black hole in our neighboring Dwarf Galaxy. According to the initial calculation of the team, this black hole structure can be between 251,000 to 1 million solar public. Its average mass will be 600,000 times the size of the sun.

Study– Which is currently in preprint but it will be published in the astrophysical Journal – the data used by the European Space Agency’s Gaia Mission, whose purpose is to map millions of stars to calculate their speed.

There may be other explanations for the event. The stars who have escaped from their galaxies can also arise from the supernova or any other strong process. Paper writers have explained, but it is not seen in the hypervelository stars that seem to have come from the large Magelic cloud.

Large Magelic Cloud is an irregular sized galaxy that orbits the Milky Way, other dwarf star clusters such as bow, carina or Draco. It has a diameter of 163,000 light years and about 14,000 light years from the earth. Astronomers believe that in the distant future – about 2.5 billion years – the larger Magelic Cloud and Milkyway will be integrated into a single larger cluster with other larger structures like Andromeda Galaxy. Experts believe that the attachment process will slow down and will not create any problems on the planet’s scale.

This story was originally attended Wired In Spanish And have been translated from Spanish.

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