Cloud formation in the atomic and molecular phase: H I self absorption (HISA) towards a giant molecular filament

Y. Wang; S. Bihr; H. Beuther; M. R. Rugel; J. D. Soler; J. Ott; J. Kainulainen; N. Schneider; R. S. Klessen; S. C. O. Glover; N. M. McClure-Griffiths; P. F. Goldsmith; K. G. Johnston; K. M. Menten; S. Ragan; L. D. Anderson; J. S. Urquhart; H. Linz; N. Roy; R. J. Smith; F. Bigiel; T. Henning; S. N. Longmore

doi:10.1051/0004-6361/201935866

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Volume 634 (February 2020)

A&A, 634 (2020) A139

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Fig. 15

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Ratio of the CNM and H₂ column densities in percentage of the Eastern region (top panel) and Western region (bottom panel). The contours in both panels indicate the integrated ¹³CO emission at levels of 5, 10, 20, and 30 K km s⁻¹.

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