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We combine our high-sensitivity southern HI survey with the Leiden/Dwingeloo Survey, considering l=240{deg}-400{deg}, b=-60{deg} to +60{deg}, and radial velocities of V=-41.8 to +40.8km/s. We point out the main HI branches surrounding the association and derive their kinematics. Kinematical HI-maps were compared with spatial maps of interstellar (IS) NaI from the literature. Upper limits for distances d were derived from optical IS absorption components from the literature. Models of expanding spherical HI shells were fitted around each stellar subgroup.</description><source format="bibcode">2010A&amp;A...512A..83P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/512/A83</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/93/211">J/ApJS/93/211 : IUE survey of HI Ly{alpha} absorption. I. (Diplas+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/404">J/AJ/124/404 : Upper Scorpius OB assoc. Lithium survey. II. 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