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tokens: We gratefully appreciate the comments from the anonymous referee that significantly improved this article. S.O. also thank Dr. Kazuya Saigo for helpful discussions. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.01025.S. ALMA is a partnership of the ESO (representing its member states), NSF (USA), and NINS (Japan), together with the 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 the ESO, AUI/NRAO, and NAOJ. This research has also made use of data from the Herschel Gould Belt Survey (HGBS) project ( http://gouldbelt-herschel.cea.fr ). The HGBS is a Herschel Key Programme jointly carried out by SPIRE Specialist Astronomy Group 3 (SAG 3), scientists of several institutes in the PACS Consortium (CEA Saclay, INAF-IFSI Rome and INAF-Arcetri, KU Leuven, and MPIA Heidelberg), and scientists of the Herschel Science Center (HSC). Data analysis was carried out in part on a common-use data analysis computer system at the Astronomy Data Center (ADC) of the National Astronomical Observatory of Japan. Facilities: ALMA , Herschel .