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tokens: This paper is based on Atacama Large Millimeter/submillimiter Array (ALMA) observations, program number 2013.1.00710.S. It makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00710.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. AZ and LAC acknowledge support from the Millennium Science Initiative (Chilean Ministry of Economy) through grant ‘Nucleus RC130007’. LAC also acknowledges support from FONDECYT-CONICYT grant #1140109. HC acknowledges support from the Spanish Ministerio de Economa y Competitividad under grant AYA2014-55840P. SP acknowledges financial support by FONDECYT grant #3140601. DAP acknowledges FONDECYT grant #3150550.