Resolving star formation with ALMA

The REsolving star formation with ALMa (REALM) project was initiated in 2015. Initially, we observed carbon monoxide (CO) in the young TMC1A protostellar system at the highest possible spatial resolution with ALMA. The obtained images showed CO and dust on spatial scales of only 6 au and revealed the presence of a disk wind. The REALM project is now being continued with the support from the Swedish research council and in 2017, we continued the long baseline observations with ALMA. The primary objectives of the research project are:

  • Constrain the launching mechanism responsible for the mass-loss observed during the earliest stages of star formation
  • Directly constrain the initial conditions for planet formation.
  • Determine how stars accrete matter.

Team members: Per Bjerkeli, Matthijs H. D. van der Wiel, Daniel Harsono, Jon Ramsey, Lars Kristensen and Jes Jørgensen.

Press clippings

Newly formed star shoots out powerful whirlwind

Researchers from the Niels Bohr Institute have used the ALMA telescopes to observe the early stages in the formation of a new solar system. For the first time they have seen how a powerful whirlwind shoot out from the rotating disc of gas and dust surrounding the young star. The results have been published in the prestigious scientific journal, Nature.

Newly formed star observed farting for the first time

For the first time, scientists have observed the powerful whirlwinds shooting out of a newly formed star located 450 light years away. The space outbursts occured in the early stages of a new solar system's formation, when young stars are known to emanate jets of gas.

Ung stjärna får hjälp av virvelvind att växa

Observationer med det stora ALMA teleskopet i Chile har gett nya inblickar i hur det kan gå till när en stjärna bildas.


Resolved images of a protostellar outflow launched by an extended disk wind
Assorted scenarios have been proposed to explain protostellar outflows; the main difference between these models is the region where acceleration of material takes place. These data show that gas is ejected from a region extending up to a radial distance of 25 astronomical units from the central protostar, and that angular momentum is removed from an extended region of the disk. This demonstrates that the outflowing gas is launched by an extended disk wind. Per Bjerkeli & Matthijs H. D. van der Wiel et al., Nature, 2016