Multi-scale analysis of the Monoceros OB 1 star-forming region - II. Colliding filaments in the Monoceros OB1 molecular cloud

Julien Montillaud; Mika Juvela; Charlotte Vastel; Jinhua He; Tie Liu; Isabelle Ristorcelli; David J. Eden; Sung-ju Kang; Kee-Tae Kim; Patrick M. Koch; Chang Won Lee; Mark G. Rawlings; Mika Saajasto; Patricio Sanhueza; Archana Soam; Sarolta Zahorecz; Dana Alina; Rebeka Bögner; David Cornu; Yasuo Doi; Johanna Malinen; Douglas J. Marshall; Elisabetta R. Micelotta; Veli-Matti Pelkonen; L. Viktor Tóth; Alessio Traficante; Ke Wang

doi:10.1051/0004-6361/201834903

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Volume 631 (November 2019)

A&A, 631 (2019) A3

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Fig. 8

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Spectra of CO, ¹³CO and C¹⁸O (J = 1–0) in the junction (left) and bridge (right) regions at the locations marked by black circles in Fig. 7. The spectra of CO is divided by 2. The black dashed lines are the 3-component Gaussian fit of the ¹³CO lines (Sect. 4.2.1).

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