PRODIGE–envelope to disk with NOEMA-IV. An infalling gas bridge surrounding two Class 0/I systems in L1448N
Context. The formation of stars has been subject to extensive studies in the past decades on
scales from molecular clouds to proto-planetary disks. It is still not fully understood how the …
scales from molecular clouds to proto-planetary disks. It is still not fully understood how the …
[HTML][HTML] Understanding the various evolutionary stages of the low-mass star-formation process by SO and SO2
SO and SO2 are two potential candidates to trace the different evolutionary phases of the
low-mass star-formation process. Here, we report observations of SO and SO2 along with …
low-mass star-formation process. Here, we report observations of SO and SO2 along with …