Hungry black hole may be cosmic 'missing link' – BBC News, BBC News

Hungry black hole may be cosmic 'missing link' – BBC News, BBC News

                                 Artwork: The presumed black hole revealed itself by tearing a star apart Image copyright                   ESA / Hubble, M. Kornmesser                                                        
Image caption                                      Artwork: The presumed black hole revealed itself by tearing apart a star that ventured too close                              

A team of astronomers has found what it says is the best evidence yet for an elusive class of black hole.

They say the presumed “intermediate-mass” black hole betrayed its existence by tearing apart a wayward star that ventured too close.

These medium-sized objects are a long-sought “missing link” in the evolution of the cosmos .

Researchers used two X-ray observatories, along with the Hubble telescope , to identify the object.

Intermediate-mass black holes are very elusive objects, and so it is critical to carefully consider and rule out alternative explanations for each candidate, said Dr Dacheng Lin, from the University of New Hampshire in Durham, US , who led the study. “That is what Hubble has allowed us to do for our candidate.”

In , Nasa’s orbiting Chandra X-ray Observatory and the European Space Agency’s XMM-Newton satellite spotted a powerful X-ray flare named 3XMM J . 4 – 01575879.

The nature of the X-ray flare meant that it could be explained by just two scenarios, according to Dr Lin. It was “either a distant (outside our galaxy) intermediate-mass black hole disrupting and swallowing a star or a cooling neutron star in our own galaxy”, he told BBC News.

Neutron stars are the crushed remnants of an exploded star.                                                                                                                         What is a black hole?

                                                                                                       Image copyright                   NASA GSFC / Jeremy Schnittman                                                        
Image caption                                      Artwork: Black holes come in different sizes, but mid-sized ones have proved elusive                              

A black hole is a region of space from which nothing, not even light, can escape

  • despite the name, they are not empty but instead consist of a huge amount of matter packed densely into a small area, giving it an immense gravitational pull
  • There is a region of space beyond the black hole called the event horizon. This is a “point of no return”, beyond which it is impossible to escape the gravitational effects of the black hole

      In order to distinguish between the two scenarios, the Hubble Space Telescope was pointed at the X-ray source to resolve its precise location. The telescope provided strong evidence that the X-rays emanated not from an isolated source in the Milky Way, but in a distant, dense star cluster on the outskirts of a different galaxy.

      This was just the type of place astronomers expected to find a mid-sized black hole. Dr Lin said the Hubble data made this the “most likely” explanation.

      So-called supermassive black holes are commonly found at the centers of galaxies; for example, our own Milky Way hosts a massive central black hole called Sagittarius A *.

                                                                                                             Image copyright                   NASA / ESA / D. LIN (UNH)                                                        
      Image caption                                      The black hole (circled) lies on the outskirts of a large galaxy                              
                                                                                                             Image copyright                   ESA                                                        
      Image caption                                      Artwork: The X-ray flare was found among thousands of observations taken by the XMM-Newton orbiting observatory                              

      But intermediate mass black holes have been particularly difficult to find because they are smaller and less active than the massive types. In addition, they don’t have as much nearby cosmic material to act as fuel, and lack the strong gravitational pull required to draw stars inwards to produce X-ray flares.

    • Astronomers effectively had to catch a mid-sized black hole red-handed in the act of gobbling up a star.

      Dr Lin and his colleagues had to comb through thousands of XMM-Newton observations to find one candidate.

      The X-ray glow from the shredded star allowed astronomers to estimate the black hole’s mass at , 10 times the mass of the Sun.

                                                                                                             Image copyright                   NASA                                                        
      Image caption                                      The Hubble Space Telescope was used for resolve the location of the X-ray source                              

      This isn’t the first candidate for a mid-sized black hole . But seeing the object tearing a star apart makes this detection the most persuasive yet, according to Dr Lin’s team.

      Intermediate-mass black holes are key to many questions about black hole evolution. For example, does a super-massive black hole grow from a mid-sized one?

      Astronomers also want to understand how mid -sized black holes form and whether they tend to reside in dense star clusters, such as this one.

      “Studying the origin and evolution of the intermediate-mass black holes will finally give an answer as to how the supermassive black holes that we find in the centers of massive galaxies came to exist, “said team member Dr Natalie Webb, from the University of Toulouse, France.

      The results are published in The Astrophysical Journal Letters. Follow Paul on Twitter.              Read More

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