RESEARCH / 01
Chaotic Mass Accretion Processes in Star Formation
Discoveries of a warped disk around L1489 IRS and multiple outflows from IRAS 15398-3359, both of which are single protostars, suggesting disk formation through chaotic mass accretion processes in turbulent environments.
Disk Structure around the Class I Protostar L1489 IRS Revealed by ALMA: A Warped-disk System Multiple Outflows around a Single Protostar IRAS 15398−3359






