Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey

V. Könyves (1, 2) , Ph. André (1) , D. Arzoumanian (3, 4) , N. Schneider (5) , A. Men’shchikov (1) , S. Bontemps (6) , B. Ladjelate (7) , P. Didelon (1) , S. Pezzuto (8) , M. Benedettini (8) , A. Bracco (9) , J. Di Francesco (10, 11) , S. Goodwin (12) , K. L. J. Rygl (13) , Y. Shimajiri (1) , L. Spinoglio (8) , D. Ward-Thompson (2) , G. J. White (14)

1 AIM (UMR7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation
2 Jeremiah Horrocks Institute for Mathematics, Physics and Astronomy [Preston]
3 Nagoya University
4 IASTRO - Instituto de Astrofísica e Ciências do Espaço
5 University of Cologne
6 LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
7 IRAM - Instituto de RadioAstronomía Milimétrica
8 IAPS - Istituto di Astrofisica e Planetologia Spaziali - INAF
9 Astrophysique
10 NRC - National Research Council of Canada
11 UVIC - University of Victoria [Canada]
12 University of Sheffield [Sheffield]
13 IRA - Istituto di Radioastronomia [Bologna]
14 RAL Space - Space Science and Technology Department [Didcot]

Keywords: submillimeter: ISM; ISM: clouds; stars: formation; ISM: individual objects: Orion B complex; ISM: structure; submillimeter: ISM

Domains: Astrophysics [astro-ph]

V. Könyves, Ph. André, D. Arzoumanian, N. Schneider, A. Men’shchikov, et al.. Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey. Astronomy and Astrophysics - A&A, 2020, 635, pp.A34. ⟨10.1051/0004-6361/201834753⟩. ⟨cea-02499010⟩