Artist impression of the young massive star Cepheus A HW2. The narrow collimated jet originates from the embryonic star which is surrounded by a dust disc as well as a larger disc of gas. The wite lines show the 3-dimensional magnetic field structure along which material falls onto the slowly rotating discs. (Image credit: Tobias Maercker). JPG version (550 kB)
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 molecular hydrogen 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 magnetic field 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 massive stars 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.
"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.
FURTHER INFORMATION
A preprint of the paper is available from http://uk.arxiv.org/abs/1002.2214
CONTACTS
Dr. Wouter Vlemmings
Argelander-Institut für Astronomie, Universität Bonn, Germany
E-mail: wouter@astro.uni-bonn.de
Tel: +49 228 733670 / 733658
Dr. Huib Jan van Langevelde
Joint Institute for VLBI in Europe, Dwingeloo, The Netherlands
E-mail: langevelde@jive.nl
Tel: +31 521 596524
Dr Robert Massey
Press and Policy Officer
Royal Astronomical Society
E-mail: rm@ras.org.uk
Tel: +44 (0)20 7734 3307
Mob: +44 (0)794 124 8035
IMAGE
An image, a movie and the relevant scientific papers are available from http://www.astro.uni-bonn.de/~wouter/papers/cepheusa/
NOTES FOR EDITORS
MERLIN
The Multi-Linked Radio Interferometer Network (MERLIN: http://www.merlin.ac.uk), operated from Jodrell Bank Observatory, is an array of seven radio telescopes distributed around the United Kingdom, with separations of up to 217km. MERLIN is operated by the University of Manchester as a National Facility of the UK Science and Technology Facilities Council.
THE ROYAL ASTRONOMICAL SOCIETY
The Royal Astronomical Society (RAS: http://www.ras.org.uk), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.
