Data for: Relations Between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud
Cite this dataset:
Wong, Tony; Hughes, A; Tokuda, K; Indebetouw, R; Onishi, T; Bandurski, J. B.; Chen, C. H. R.; Fukui, Y; Glover, S. C. O.; Klessen, R. S.; Pineda, J. L.; Roman-Duval, J.; Sewilo, M.; Wojciechowski, E.; Zahorecz, S. (2019): Data for: Relations Between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud. University of Illinois at Urbana-Champaign. https://doi.org/10.13012/B2IDB-7090706_V1
Use this persistent URL to link to this dataset:
Dataset Description

12CO and 13CO maps for six molecular clouds in the Large Magellanic Cloud, obtained with the Atacama Large Millimeter/submillimeter Array (ALMA). See the associated article in the Astrophysical Journal, and README files within each ZIP archive. Please cite the article if you use these data.
Subject Physical Sciences
Keywords Radio astronomy
License CC0
Funder JAO.ALMA [Cycle 4]-Grant:2016.1.00193.S
Corresponding Creator Tony Wong
Downloaded 617 times
Version DOI Comment Publication Date
1 10.13012/B2IDB-7090706_V1 2019-09-25
Open in Globus File Manager what's this?
1.1 KB File
2.44 KB File
487 Bytes File
1.11 GB File
3.18 GB File
8.7 KB File

Contact the Research Data Service for help interpreting this log.

Dataset update: {"subject"=>["Life Sciences", "Physical Sciences"]} 2019-09-25T15:31:18Z