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

V. Könyves; Ph. André; D. Arzoumanian; N. Schneider; A. Men’shchikov; S. Bontemps; B. Ladjelate; P. Didelon; S. Pezzuto; M. Benedettini; A. Bracco; J. Di Francesco; S. Goodwin; K. L. J. Rygl; Y. Shimajiri; L. Spinoglio; D. Ward-Thompson; G. J. White

doi:10.1051/0004-6361/201834753

Journal articles

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

* Corresponding author

1 AIM (UMR_7158 / 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

LPENS - Laboratoire de physique de l'ENS - ENS Paris

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

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Journal articles

Domain :

Physics [physics] / Astrophysics [astro-ph]

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

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

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