An international team of researchers from multiple institutions, including INRS, is shedding light on the mystery of matter accretion in young stars. Published in the November 1, 2017 Science Advances online journal, their discovery helps explain how matter accumulates on the surface of a young star and reconciles the theory behind and observations on the accretion process - a matter of debate among astrophysicists because of the limited number of theoretical models and actual observations.

An experiment replicating the accretion phenomenon on a star was conducted in a laboratory. Researchers took a close look at what happens when a laser-produced column of plasma impacts a solid obstacle in the presence of an intense magnetic field.

X-ray emissions measurements verified the presence of an envelope of plasma around the core of the accretion zone of the matter on the star's surface. Discovery of the envelope allows researchers to accurately calculate the matter accretion rate.

The importance of this discovery lies in the fact that a star is born, grows, reaches adult size, and then dies either by exploding or by collapsing in on itself to have much less volume but much greater density.

Stars have a lifespan like any living thing. The adult phase - like our sun is in - lasts for many billions of years. Outside the birth of a planet (like Earth) or the appearance of life, it is a relatively quiet time in the life of a star.

Physicists are more interested in the birth and death of stars - these are defining moments. By looking at the emission of x-rays from the surface, scientists can also determine the rate at which stars grow under the influence of gravity as they pull in the interstellar matter surrounding them.

To accurately interpret these x-rays, scientists must ensure they are not being obscured by something - hence the importance of the discovery of an envelope.

Research paper

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Sao Paulo, Brazil (SPX) Nov 03, 2017
A group of Brazilian astronomers observed a pair of celestial objects rarely seen in the Milky Way: a very low-mass white dwarf and a brown dwarf. A white dwarf is the endpoint of the evolution of an intermediate- or low-mass star, with a mass between 0.5 and 8 times that of our Sun. A brown dwarf is a substellar object with mass intermediate between those of a star and a planet. On analyz ... read more

Related Links
Institut national de la recherche scientifique - INRS
Stellar Chemistry, The Universe And All Within It

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