Massive stars' magnetically controlled diets

Feb 18, 2010 by Robert Massey
rtist’s impression of the young massive star Cepheus A HW2. The narrow collimated jet originates from the embryonic star which lies at the centre of the image, hidden within a surrounding dust disc and larger disc of gas. The white lines indicate the 3-dimensional magnetic field structure along which material falls onto the slowly rotating discs. Credit: Tobias Maercker

( -- A team of astronomers, led by Dr. Wouter Vlemmings at Bonn University, has used the MERLIN radio telescope network centred on the Jodrell Bank Observatory to show that magnetic fields play an important role during the birth of massive stars. Magnetic fields are already known to strongly influence the formation of lower-mass stars like our Sun. This new study reveals that the way in which high-mass and low-mass stars form may be more similar than previously suspected. The scientists report their work in the journal Monthly Notices of the Royal Astronomical Society.

Massive stars, more than 8 times the mass of the Sun, are crucial to the formation of other stars, planets and even life. Though rare, they dominate the content and evolution of the interstellar material in the Galaxy and are responsible for the production of heavy elements such as iron. However, the question of how massive stars are formed has proved extremely difficult to answer. The role of magnetic fields in particular has been a topic of great debate. Many scientists thought that radiation and turbulence would be the more dominant factors, and hence their formation process would be significantly different from that of less massive stars such as our Sun.

"While magnetic fields have been observed in the clouds of from which stars form, observations close to massive stars have up to now been in short supply," says Vlemmings. “If the formation of massive stars is similar to their lighter counterparts, we should be able to detect the strong magnetic fields needed to both produce the jets and stabilize the disks associated with them.”

For the first time, Wouter Vlemmings and his collaborators have managed to observe the 3-dimensional structure around the disk of the massive newly forming star (or protostar) Cepheus A HW2. At a distance of 2300 light years from the Sun, Cepheus A is one of the nearest regions where form and earlier observations of this region revealed the presence of a disk from which the gas falls on to HW2. In their new observations, the astronomers have found that the magnetic field is surprisingly regular and strong, implying that it is controlling how the matter is transferred through the disk to feed the growing embryonic star.

Animation (click 'Enlarge') of the observations and the Cepheus A HW2 magnetic field. The spheres indicate velocity labelled methanol maser regions and the vectors indicate the 3-dimensional field direction determined for these masers. The thin and thick grey structures are the gas and dust disks respectively. The collimated radio outflows are indicated by the blue and red cones.

"Our new technique allows us for the first time to measure the 3D structure of the magnetic field around a massive protostar. We can see that its structure is surprisingly similar to how we think the field looks when much smaller stars form," adds co-author Huib Jan van Langevelde, director of the Joint Institute for Very Long BaseIine Interferometry in Europe (JIVE).

To determine the magnetic field structure, the researchers used the MERLIN telescope array to observe radio waves (with a wavelength of approximately 5 cm) that are amplified by methanol molecules. These methanol molecules, the simplest of the alcohol compounds, are found in regions surrounding the massive disk around HW2, which extend over a region 10 times the size of our Solar System. Such regions are called masers, because they amplify microwave radiation in the same way a laser amplifies light radiation. Even though a strong magnetic field produces only a very weak signature in the signal from the methanol molecules, this amplification is strong enough to make the new work possible.

These new observations will be a cornerstone of one of the first major scientific legacy projects to be carried out with the new e-MERLIN radio telescope network. e-MERLIN is a major upgrade to the MERLIN network that made it 10 times more sensitive. The legacy project, of which Dr. Vlemmings is one of the lead scientists, will use the unique capabilities of the upgraded network to reveal both the magnetic field and the immediate surroundings of many massive protostars of different ages.

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More information: A preprint of the paper is available from

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User comments : 4

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1 / 5 (4) Feb 18, 2010
Welcome to the Electric Universe. We've been expecting you.
1 / 5 (3) Feb 18, 2010
What's unscientific about doing research, forming theories, making predictions and then testing those predictions against the data?

The theory is that magnetic fields play a greater role than "gravity" in the formation of stars of all scales. This is understood because stars are the focal points of electric currents, just not a random collection of particles collapsing upon themselves for no reason.

Interestingly enough, Star formation relies heavily upon the "virial theorem" which, has already been extended to include electric and magnetic fields. Even more entertaining is the fact that the equation is used to model "plasmoids".

And sorry, if you can't see an analog between plasmoids and stars...

If your scope of the Electric Universe is a Google Video documentary, then your ignorance is only outweighed by your hostility.
1 / 5 (3) Feb 19, 2010
This seems reasonable to me.

Other stars probably formed as the Sun did, on the highly magnetic, collapsed, energetic core of the supernova that gave birth to the solar system.

Oliver K. Manuel
3 / 5 (2) Feb 20, 2010
Dr. Manuel, how plausible is it that a 'dark' plasmoid with a mass of 3.6 million solar masses is hiding at the center of the Milky Way galaxy while quintillions of stellar and substellar mass plasmoids are also presumably abundant yet outshine the supermassive plasmoid that is Sagittarius A*? How do you account for the production of multiwavelength radiation in exact accordance to that measured from Sagittarius A* (e.g flickering) and at the same time explicitly account for the time variability of said radiation.?

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