Massive and low-mass protostars in massive "starless" cores
The
infrared dark clouds (IRDCs) G11.11$-$0.12 and G28.34$+$0.06 are two of
the best-studied IRDCs in our Galaxy. These two clouds host clumps at
different stages of evolution, including a massive dense clump in both
clouds that is dark even at 70 and 100$μ$m.
https://arxiv.org/abs/1901.07582
No comments:
Post a Comment