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Flickering ribbons shield star-forming gas
Posted: 16 March 2010

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By all rights massive stars should emerge from their nebulous wombs stillborn, as their radiation heats the surrounding gas and stops the star from growing. Now new research has revealed that spiral filaments of gas act as a shield, absorbing the heat of young stars and allowing gas from beyond to continue to fall onto them.

All baby stars have a ‘switching on’ point. Initially, as they condense out of a cloud of molecular hydrogen, they generate energy via gravitational collapse, but after a million years or so into their protracted birth their core temperatures become hot enough to ignite nuclear fusion reactions, and a real star is born.

The Trifid Nebula in infrared light, an incubator to a single massive, but still growing, star, surrounded by 30 much smaller embryonic stars. Image: NASA/JPL–Caltech/J Rho (SSC/Caltech).

For lower mass stars such as the Sun this is not a problem – by the time they switch on they are just about done growing anyway. The most massive stars do face a problem however; as the nuclear fusion process begins within them, they are still growing from the accumulation of infalling gas. The star’s ultraviolet radiation should heat and ionise the surrounding gas, blowing it away on its stellar wind and preventing the star from growing further. How then do the most massive stars form?

This puzzle has now been solved by a team of astronomers from the United States, Germany and Mexico. Using supercomputers at the Texas Advanced Computing Center and the Leibniz and Juelich Computing Centres in Germany, they modelled how gas would behave around a young massive star. They found that the gas does not fall evenly onto the star, but that over-densities form filamentary concentrations of gas, like immense spiral ribbons that gradually wind onto the star. These ribbons can absorb much of the young star’s radiation, shielding the rest of the nebula. The variation in these ribbons can cause the innermost regions to flicker like a candle over the course of hundreds of thousands, or even millions, of years.

Recent studies have shown how magnetic fields play a major role in attracting gas onto a massive star along field lines (read our related news story here), and the team are currently performing simulations to measure the role of magnetic fields within the ribbons. However, team member Mordecai-Mark Mac Low of the American Museum of Natural History says that initial results indicate that magnetic fields do not have an effect on the formation of the radiation-absorbing ribbons. “For very massive systems, magnetic fields are likely to be far too weak to fight self gravity,” he tells Astronomy Now. However, magnetic fields may still be important in gathering in the material from the wider interstellar medium in the first place.

The Planets
From tiny Mercury to distant Neptune and Pluto, The Planets profiles each of the Solar System's members in depth, featuring the latest imagery from space missions. The tallest mountains, the deepest canyons, the strongest winds, raging atmospheric storms, terrain studded with craters and vast worlds of ice are just some of the sights you'll see on this 100-page tour of the planets.

Hubble Reborn
Hubble Reborn takes the reader on a journey through the Universe with spectacular full-colour pictures of galaxies, nebulae, planets and stars as seen through Hubble's eyes, along the way telling the dramatic story of the space telescope, including interviews with key scientists and astronauts.

3D Universe
Witness the most awesome sights of the Universe as they were meant to be seen in this 100-page extravaganza of planets, galaxies and star-scapes, all in 3D!


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