Resolving star and planet formation with ALMA
Paper i proceeding, 2020

Disks around young stars are the sites of planet formation. As such, the physical and chemical structure of disks have a direct impact on the formation of planetary bodies. Outflowing winds remove angular momentum and mass and affect the disk structure and therefore potentially planet formation. Until very recently, we have lacked the facilities to provide the necessary observational tools to peer into the wind launching and planet forming regions of the young disks. Within the framework of the Resolving star formation with ALMA program, young protostellar systems are targeted with ALMA to resolve the disk formation, outflow launching and planet formation. This contribution presents the first results of the program. The first resolved images of outflow launching from a disk were recently reported towards the Class I source TMC1A (Bjerkeli et al. 2016) where we also present early evidence of grain growth (Harsono et al. 2018).

ISM: Jets and outflows

Stars: Formation


Protoplanetary disks

Stars: Winds


Per Bjerkeli

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

D. Harsono

Universiteit Leiden

M. H. D. van der Wiel

Netherlands Institute for Radio Astronomy (ASTRON)

Jon P Ramsey

University of Virginia

L. Kristensen

Niels Bohr Institute

Jes K. Jørgensen

Niels Bohr Institute

Proceedings of the International Astronomical Union

1743-9213 (ISSN) 1743-9221 (eISSN)

Vol. 14 106-110

IAU Symposium 345
Wien, Austria,


Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik



Mer information

Senast uppdaterat