Artist’s conception shows a zoomed in view of the mystery of MWC 349A and its surrounding disc of gas and dust that are being shaped by the winds and high-speed jet. © ALMA (ESO/ NAOJ/ NRAO), M Weiss (NRAO/ AUI/ NSF).
Astronomers consider magnetic forces at play as they discover superfast jet launching from star’s gas disc at ‘impossibly high speeds’
While using the Atacama Large Millimeter/submillimeter Array (ALMA) to study the masers around oddball star MWC 349A scientists discovered something unexpected; a previously unseen jet of material launching from the star’s gas disc at impossibly high speeds. What’s more, they believe the jet is caused by strong magnetic forces surrounding the star.
The discovery could help researchers to understand the nature and evolution of massive stars and how hydrogen masers are formed in space.
Located roughly 3,900 light-years away from Earth in the constellation Cygnus, MWC 349A’s unique features make it a hot spot for scientific research in optical, infrared, and radio wavelengths.
The massive star – roughly 30 times the mass of the sun – is one of the brightest radio sources in the sky, and one of only a handful of objects known to have hydrogen masers.
These masers amplify microwave radio emissions, making it easier to study processes that are typically too small to see. It is this unique feature that allowed scientists to map MWC 349A’s disc in detail for the first time.
Sirina Prasad, an undergraduate research assistant at the Center for Astrophysics | Harvard & Smithsonian (CfA), and the primary author of the paper, said: “A maser is like a naturally occurring laser; it’s an area in outer space that emits a really bright kind of light.
“We can see this light and trace it back to where it came from, bringing us one step closer to figuring out what’s really going on.”
See also: Superfast jet result of collision between two neutron stars
The massive star MWC 349A is one of the brightest radio sources in the sky. But, at 3,900 light-years away from Earth, scientists needed help to see what’s really going on, and in this case, to discover a jet of material blasting out from the star’s gas disc at 500 km/s. Previously hidden amongst the winds flowing out from the star, the jet was discovered using the combined resolving power of ALMA’s Band 6 (right) and Band 7 (left), and hydrogen masers— naturally occurring lasers that amplify microwave radio emissions, shown here in this ALMA science image. The revelation may help scientists to better understand the nature and evolution of massive stars. © ALMA (ESO/ NAOJ/ NRAO), S Prasad/ CfA.
magnetic force
Leveraging the resolving power of ALMA’s Band 6, developed by the US National Science Foundation’s National Radio Astronomy Observatory (NRAO), the team was able to use the masers to uncover the previously unseen structures in the star’s immediate environment.
Qizhou Zhang, a senior astrophysicist at CfA, and the project’s principal investigator added: “We used masers generated by hydrogen to probe the physical and dynamic structures in the gas surrounding MWC 349A and revealed a flattened gas disc with a diameter of 50au, approximately the size of the solar system, confirming the near-horizontal disc structure of the star. We also found a fast-moving jet component hidden within the winds flowing away from the star.”
The observed jet is ejecting material away from the star at a blistering 500km per second. According to researchers, it is probable that a jet moving this fast is being launched by a magnetic force.
In the case of MWC 349A, that force could be a magnetohydrodynamic wind – a type of wind whose movement is dictated by the interplay between the star’s magnetic field and gases present in its surrounding disc.
Collimated jet
Prasad said: “Our previous understanding of MWC 349A was that the star was surrounded by a rotating disc and photo-evaporating wind. Strong evidence for an additional collimated jet had not yet been seen in this system.
“Although we don’t yet know for certain where it comes from or how it is made, it could be that a magnetohydrodynamic wind is producing the jet, in which case the magnetic field is responsible for launching rotating material from the system.
“This could help us to better understand the disc-wind dynamics of MWC 349A, and the interplay between circumstellar discs, winds, and jets in other star systems.”
The observations were presented at the 241st meeting of the American Astronomical Society (AAS) in Seattle, Washington.
