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Star formation is observed to be strongly correlated to dense regions of molecular gas. Although the exact nature of the link between star formation and molecular hydrogen is still unclear, some have suggested that shielding of dense gas by dust grai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b446d58548a99fae5d088c791b2fe853
Publikováno v:
Astrophysical Journal; 2/1/2019, Vol. 871 Issue 2, p1-1, 1p
