A Detailed Analysis of the Cloud Structure and Dynamics in Aquila Rift

We present maps in several molecular emission lines of a 1 square degree region covering the W40 and Serpens South molecular clouds belonging to the Aquila Rift complex. The observations were made with the 45 m telescope at the Nobeyama Radio Observatory. We found that the 12CO and 13CO emission lin...

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Veröffentlicht in:	The Astrophysical journal 2020-06, Vol.895 (2), p.137
Hauptverfasser:	Shimoikura, Tomomi, Dobashi, Kazuhito, Hatano, Yoshiko, Nakamura, Fumitaka
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Cloud structure Dynamic structural analysis Emission Emission lines Emissions H II regions Interstellar medium Molecular clouds Spatial distribution Star & galaxy formation Star formation Stellar winds
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