The Hubble Space Telescope is tracking down a
suspected black hole that shredded a wayward star that came too close for
comfort.
Background
The famed space observatory made the find while hunting down
the source of a powerful burst of X-rays caught in 2006 by two other cosmic
telescopes: NASA's Chandra X-ray Observatory and the European Space
Agency's X-ray Multi-Mirror Mission (XMM-Newton) .
Details
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At the time, astronomers weren't sure if the
X-rays had come from inside or outside of the Milky Way galaxy, but new
high-resolution photography by Hubble shows that the X-ray source (known as
3XMM J215022.4−055108) is located in a star cluster at the edge of another
galaxy.
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The team's work further suggests the star
cluster may have been the core of a small dwarf galaxy disrupted long ago, when
the dwarf galaxy strayed too close to the larger galaxy that currently hosts
the star cluster.
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Gravitational interactions with the larger
galaxy may have ripped the dwarf galaxy apart, leaving only a small cluster of
stars in its wake.
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In much the same way, astronomers believe that
the gravitational pull of the black hole inside this cluster shredded a star
that got too close, thereby producing the X-ray flare detected in 2006.
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IMBHs have been particularly difficult to find
because they are smaller and less active than supermassive black holes; they do
not have readily available sources of fuel, nor as strong a gravitational pull
to draw stars and other cosmic material which would produce telltale X-ray
glows.
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IMBHs are believed to be a "missing link"
in our understanding of how black holes evolve. Astronomers have seen
many examples of small black holes that are similar in size to a star, and
other examples of much larger black holes that typically reside in the centers
of galaxies.
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But IMBHs remain difficult to
confirm as astronomers struggle to understand how supermassive black holes
got so big, compared to stellar-sized black holes.
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Hubble also helped track down another possible
IMBH in 2009. The object, called HLX-1, was spotted on the edge of a
galaxy known as ESO 243-49, and also resides in a star cluster that could have
been a dwarf galaxy in the ancient past.
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