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The Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN. I. Catalog of Molecular Clouds

  • Authors: Y. Fukui, A. Kawamura, T. Minamidani, Y. Mizuno, Y. Kanai, N. Mizuno, T. Onishi, Y. Yonekura, A. Mizuno, H. Ogawa, and M. Rubio

Fukui et al. 2008 The Astrophysical Journal Supplement Series 178 56.

  • Provider: AAS Journals

Caption: Fig. 13.

Cumulative mass spectra of the MCO of the 230 GMCs. The best‐fitting power law to MCO above the completeness limit ﹩5\times 10^{4}﹩ M (thick vertical line) is ﹩N_{\mathrm{cloud}\,}( \geq M_{\mathrm{CO}\,}) =6.6\times 10^{5}M^{-0.75\pm 0.06}-3.4﹩ and is indicated by a dashed line. The dotted line indicates the best‐fitting power law, ﹩N_{\mathrm{cloud}\,}( \geq M_{\mathrm{CO}\,}) =1.3\times 10^{8}M^{-1.2\pm 0.2}-0.72﹩, obtained by fitting MCO of the 47 clouds with ﹩M_{\mathrm{CO}\,}\geq 3\times 10^{5}﹩ M (thin vertical line).

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