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

Home

All issues

Volume 634 (February 2020)

A&A, 634 (2020) A139

Full HTML

Open Access

Fig. 12

Open with DEXTER Download original image

Histograms of the FWHM linewidth of the HISA and ¹³CO emission in black (thin) and red (thick), respectively. Left and middle panels: all extracted pixels within the marked eastern (around l = 36.5°) and western (around l = 34°) polygon inFig. 14. Right panel: all extracted pixels for the whole filament (red polygon in Fig. 14).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.