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The Gaia Collaboration has used Gaia-DR2 sources with six-dimensional (6D) phase space information to derive kinematical maps within 5 kpc of the Sun, which is a reachable range for stars with relative error in distance lower than 20%.\n  AIMS. Here we aim to extend the range of distances by a factor of two to three, thus adding the range of Galactocentric distances between 13 kpc and 20 kpc to the previous maps, with their corresponding error and root mean square values.\n  METHODS. We make use of the whole sample of stars of Gaia-DR2 including radial velocity measurements, which consi","authors_text":"F. Sylos Labini, M. Lopez-Corredoira","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-10-31T17:50:55Z","title":"Gaia-DR2 extended kinematical maps. 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