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2019ApJ...886...14F - Astrophys. J., 886, 14-14 (2019/November-3)
An ALMA view of molecular filaments in the Large Magellanic Cloud. I. The formation of high-mass stars and pillars in the N159E-Papillon Nebula triggered by a cloud-cloud collision.
FUKUI Y., TOKUDA K., SAIGO K., HARADA R., TACHIHARA K., TSUGE K., INOUE T., TORII K., NISHIMURA A., ZAHORECZ S., NAYAK O., MEIXNER M., MINAMIDANI T., KAWAMURA A., MIZUNO N., INDEBETOUW R., SEWILO M., MADDEN S., GALAMETZ M., LEBOUTEILLER V., CHEN C.-H.R. and ONISHI T.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): ISM: clouds - ISM: individual: N159E - ISM: kinematics and dynamics - stars: formation - stars: protostars
Nomenclature: Fig. 1: [FTS2019] N159E MMS-N (Nos MMS-1 to MMS-2).
CDS comments: MMS-1 and MMS-2 are not in SIMBAD.
Simbad objects: 15
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