dc.contributor.author | Kirk, H | |
dc.contributor.author | Johnstone, D | |
dc.contributor.author | Di Francesco, J | |
dc.contributor.author | Lane, J | |
dc.contributor.author | Buckle, J | |
dc.contributor.author | Berry, DS | |
dc.contributor.author | Broekhoven-Fiene, H | |
dc.contributor.author | Currie, MJ | |
dc.contributor.author | Fich, M | |
dc.contributor.author | Hatchell, J | |
dc.contributor.author | Jenness, T | |
dc.contributor.author | Mottram, JC | |
dc.contributor.author | Nutter, D | |
dc.contributor.author | Pattle, K | |
dc.contributor.author | Pineda, JE | |
dc.contributor.author | Quinn, C | |
dc.contributor.author | Salji, C | |
dc.contributor.author | Tisi, S | |
dc.contributor.author | Hogerheijde, MR | |
dc.contributor.author | Ward-Thompson, D | |
dc.date.accessioned | 2016-08-09T15:30:23Z | |
dc.date.issued | 2016-04-18 | |
dc.description.abstract | © 2016. The American Astronomical Society. All rights reserved.The James Clerk Maxwell Telescope Gould Belt Legacy Survey obtained SCUBA-2 observations of dense cores within three sub-regions of Orion B: LDN 1622, NGC 2023/2024, and NGC 2068/2071, all of which contain clusters of cores. We present an analysis of the clustering properties of these cores, including the two-point correlation function and Cartwright's Q parameter. We identify individual clusters of dense cores across all three regions using a minimal spanning tree technique, and find that in each cluster, the most massive cores tend to be centrally located. We also apply the independent M- technique and find a strong correlation between core mass and the local surface density of cores. These two lines of evidence jointly suggest that some amount of mass segregation in clusters has happened already at the dense core stage. | en_GB |
dc.description.sponsorship | The JCMT has historically been operated by the
Joint Astronomy Centre on behalf of the Science and
Technology Facilities Council of the United Kingdom, the
National Research Council of Canada and the Netherlands
Organisation for Scientific Research. Additional funds for the
construction of SCUBA-2 were provided by the Canada
Foundation for Innovation. The authors thank the JCMT staff
for their support of the GBS team in data collection and
reduction efforts. The Starlink software (Currie et al. 2014) is
supported by the East Asian Observatory. This research used
the facilities of the Canadian Astronomy Data Centre operated
by the National Research Council of Canada with the support
of the Canadian Space Agency | en_GB |
dc.identifier.citation | Astrophysical Journal, 2016, Vol. 821, Number 2 | en_GB |
dc.identifier.doi | 10.3847/0004-637X/821/2/98 | |
dc.identifier.uri | http://hdl.handle.net/10871/22939 | |
dc.language.iso | en | en_GB |
dc.publisher | American Astronomical Society | en_GB |
dc.rights | This is the final version of the article. Available from the American Astronomical Society via the DOI in this record. | en_GB |
dc.title | The JCMT Gould Belt Survey: dense core clusters in Orion B | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2016-08-09T15:30:23Z | |
dc.identifier.issn | 0004-637X | |
dc.identifier.journal | Astrophysical Journal | en_GB |