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AstroBlogs.ru | 23 2013 10:45
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Artist concept of a brown dwarf, spotted by NASA’s Spitzer Space Telescope, surrounded by a spinning protoplanetary disk. UC Berkeley researchers have developed a model that shows how vortices help destabilize the disk so that gas can spiral inward toward a forming star. (Image courtesy of NASA/JPL-Caltech)

A new theory from researchers at UC Berkeley explains how “zombie vortices” help lead to the birth of a new star.

New-Theory-Shows-How-Zombie-Vortices-Play-Role-in-Starbirth (700x560, 288Kb)

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Illustration of a protoplanetary disk based upon observations from the Keck II telescope. (Image courtesy of W. M. Keck Observatory).

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Binary star formation through disk fragmentation starts (left) with a young star surrounded by a rotating disk of gas and dust. The disk fragments under its own gravity, with a second star forming within the disk (center), surrounded by its own disk. At right, the two stars form an orbiting pair. 100 Astronomical Units (AU) is roughly the diameter of our Solar System. (full image) Credit: Bill Saxton, NRAO/AUI/NSF

New research from the Karl G. Jansky Very Large Array makes disk fragmentation the strongest explanation for how close multiple star systems are formed.

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