Gas distribution around the trinary protostars IRAS 04239+2436 (IMAGE)
Caption
Gas distribution around the trinary protostars IRAS 04239+2436, (left) ALMA observations of SO emissions, and (right) as reproduced by the numerical simulation on the supercomputer ATERUI. In the left panel, protostars A and B, shown in blue, indicate the radio waves from the dust around the protostars. Within protostar A, two unresolved protostars are thought to exist. In the right panel, the locations of the three protostars are shown by the blue crosses.
Credit
ALMA (ESO/NAOJ/NRAO), J.-E. Lee et al.
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License
Original content