Cluster formation in the W 40 and Serpens South complex triggered by the expanding H ii region
We present the results of mapping observations covering a large area of 1 square degree around W 40 and Serpens South carried out in the 12CO (J = 1–0), 13CO (J = 1–0), C18O (J = 1–0), CCS (JN = 87–76), and N2H+ (J = 1–0) emission lines with the 45 m Nobeyama Radio Telescope. W 40 is a blistered H i...
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Veröffentlicht in: | Publications of the Astronomical Society of Japan 2019-12, Vol.71 (Supplement_1) |
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Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
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