Fragmentation, rotation, and outflows in the high-mass star-forming region IRAS 23033+5951 - A case study of the IRAM NOEMA large program CORE

F. Bosco; H. Beuther; A. Ahmadi; J. C. Mottram; R. Kuiper; H. Linz; L. Maud; J. M. Winters; T. Henning; S. Feng; T. Peters; D. Semenov; P. D. Klaassen; P. Schilke; J. S. Urquhart; M. T. Beltrán; S. L. Lumsden; S. Leurini; L. Moscadelli; R. Cesaroni; Á. Sánchez-Monge; A. Palau; R. Pudritz; F. Wyrowski; S. Longmore

doi:10.1051/0004-6361/201935318

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Volume 629 (September 2019)

A&A, 629 (2019) A10

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Fig. 10

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Herschel/PACS observations at 160 μm towards IRAS 23033+5951 and IRAS 23031+5948, from the Hi-GAL survey (Molinari et al. 2010).

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