Massive Stars Are Formed Not From Dust Disk but From Debris – “A Chaotic Mess”

Artist’s impression of the gas-rich debris disk.
Credit: NAOJ

A Dutch-led team of astronomers has discovered that high-mass stars are formed differently from their smaller siblings. Whereas small stars are often surrounded by an orderly disk of dust and matter, the supply of matter to large stars is a chaotic mess. The researchers used the Atacama Large Millimeter/submillimeter Array (ALMA) telescope for their observations, and recently published their findings in the Astrophysical Journal.

It is well known how small, young stars are created. They accrete matter from a disk of gas and dust in a relatively orderly fashion. Astronomers have already seen many of these disks of dust around young, low-mass stars but never around young, high-mass stars. This raised the question of whether large stars come into existence in the same way as small ones.

Large stars are formed in a different way

“Our findings now provide convincing evidence to show that the answer is ‘No,’” according to Ciriaco Goddi, affiliated with the ALMA expertise center Allegro at Leiden University and with Radboud University in Nijmegen.

Goddi led a team that studied three young, high-mass stars in star-forming region W51, roughly 17,000 light years from Earth. The researchers were looking in particular for large, stable disks expelling jets of matter perpendicular to the surface of the disk. Such disks should be visible with the high resolution ALMA telescopes.

Not stable disks but chaos

Goddi: “But instead of stable disks, we discovered that the accretion zone of young, high-mass stars looks like a chaotic mess.”

The observation showed strands of gas coming at the young, high-mass stars from all directions. In addition, the researchers saw jets which indicate that there may be small disks, invisible to the telescope. Also, it would appear that some hundred years ago the disk around one of three stars studied rotated. In short: chaos.

Matter from multiple directions

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