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Shedding light on the growth of stars and black holes

Posted October 15, 2015

A Southampton astronomer is among a team of international researchers whose work has revealed a surprising similarity between the way in which astronomical objects grow including black holes, white dwarfs and young stars.

Scale diagram of astronomical objects. Image credit: Simone Scaringi

Scale diagram of astronomical objects. Image credit: Simone Scaringi

Christian Knigge, Professor in Physics and Astronomy, worked with colleagues from around the world to study one of the most important, but least understood processes in astronomy – accretion, where the mass of an object grows by gravitationally collecting material from nearby.

The article Accretion-induced variability links young stellar objects, white dwarfs, and black holes has been published in the latest edition of the journal Science Advances.

The paper reveals a close relationship between the way in which different types of accreting objects vary in brightness over time. Their results connect proto-stars resembling our Sun at the time of its birth, to accreting white dwarfs, to supermassive black holes with a billion times the mass of the Sun, located in galaxies millions of light years away.

The team found that the two most important properties of the object are its physical size, scale and the rate at which it is accreting matter. They discuss a unified scenario for understanding brightness variations from accretion discs around different types of stars and compact objects. Previous work had unified the variability in discs around black holes of different mass ranges, but by considering not just the mass of the object, but also its size, scientists can now add accreting white dwarfs and proto-stars to this unified picture.

Professor Knigge said: “This is a really exciting result. It suggests that the process by which astronomical objects grow is fundamentally the same, regardless of the type, mass or size of the object.”

Source: The University of Southampton

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