A swarm of black holes could explain Galactic fluffiness

Artist’s impression of stellar-mass black hole

Although black holes (left, surrounded by a disc of hot gas; artist’s impression) often consume matter from stars, their gravity can also fling stars outwards. Credit: ESA, NASA and Felix Mirabel

Astronomy and astrophysics

A swarm of black holes could explain Galactic fluffiness

Diffuse Milky Way formation might have been depleted by star-hurling black holes.

An ancient star cluster’s long ‘tails’ of stars seems to be the handiwork of an unseen clutch of black holes: their gravitational tugs fling stars outwards, and Galactic forces then pull the stars farther out.

Astronomers classify the group of stars called Palomar 5 as a globular cluster, a roughly spherical collection of old stars. Located some 20,000 parsecs from Earth, Palomar 5 is among the ‘fluffiest’ — or least dense — of the Milky Way’s globular clusters. But Mark Gieles at the University of Barcelona in Spain and his colleagues say the evidence suggests that the cluster was once much denser.

The researchers modelled how a variety of star clusters with Palomar 5’s orbit would evolve over a period of 11.5 billion years. The starting points that evolved into the best matches for Palomar 5 and its stellar tail were clusters in which black holes formed and stuck around, their gravity helping to push stars out to create the fluffy cluster we see today.

One billion years from now, the team’s work suggests, Palomar 5 will have jettisoned all of its stars; only black holes will remain.

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