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Data for: Relations Between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud

  • Tony Wong (Creator)
  • A Hughes (Creator)
  • K Tokuda (Creator)
  • R Indebetouw (Creator)
  • T. Onishi (Creator)
  • J. B. Bandurski (Creator)
  • C. H.R. Chen (Creator)
  • Y. Fukui (Creator)
  • S. C. O. Glover (Creator)
  • R. S. Klessen (Creator)
  • J. L. Pineda (Creator)
  • J. Roman-Duval (Creator)
  • M. Sewilo (Creator)
  • E. Wojciechowski (Creator)
  • S. Zahorecz (Creator)

Dataset

Description

<sup>12</sup>CO and <sup>13</sup>CO 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.
Date made availableSep 25 2019
PublisherUniversity of Illinois Urbana-Champaign

Keywords

  • Radio astronomy

  • Relations between Molecular Cloud Structure Sizes and Line Widths in the Large Magellanic Cloud

    Wong, T., 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., Sewiło, M., Wojciechowski, E. & Zahorecz, S., Nov 1 2019, In: Astrophysical Journal. 885, 1, 50.

    Research output: Contribution to journal › Article › peer-review

    Open Access

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