We investigate whether the Lupus I molecular could have formed in a colliding flow, and in particular, how the kinematics of the cloud might have been influenced by the larger scale gas dynamics. Lupus I cloud is found between the Upper Scorpius (USco) and Upper Centaurus-Lupus (UCL) subgroups of the Scorpius-Centaurus OB association, where the expanding USco H I shell appears to interact with a bubble currently driven by the winds of the remaining B stars of UCL.Īims. Fermi 5, 50125 Firenze, Italyģ Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, GermanyĤ Excellence Cluster Universe, Boltzmannstrasse 2, 85748 Garching, Germanyĥ School of Mathematics & Physics, Private Bag 37, University of Tasmania, Hobart 7001, AustraliaĦ Centre for Astrophysics Research, School of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UKĬontext. 1, 81679 München, GermanyĮ-mail: INAF–Osservatorio Astrofisico di Arcetri, L.go E. Preibisch 1ġ Universitäts-Sternwarte München, Ludwig-Maximilians-Universität, Scheinerstr. Astronomical objects: linking to databasesī. Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes
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