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)
Hauptverfasser: Shimoikura, Tomomi, Dobashi, Kazuhito, Nakamura, Fumitaka, Shimajiri, Yoshito, Sugitani, Koji
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Sprache:eng
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