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Massive Outflows Associated with ATLASGAL Clumps

  • Authors: A. Y. Yang, M. A. Thompson, J. S. Urquhart, and W. W. Tian

2018 The Astrophysical Journal Supplement Series 235 3.

  • Provider: AAS Journals

Caption: Figure 4.

Detection rate as a function of clump mass ﹩{M}_{\mathrm{clump}}({M}_{\odot })﹩, bolometric luminosity of central objects ﹩{L}_{\mathrm{bol}}({L}_{\odot })﹩, luminosity-to-mass ratio ﹩{L}_{\mathrm{bol}}/{M}_{\mathrm{clump}}({L}_{\odot }/{M}_{\odot })﹩, and peak H2 column density of clumps ﹩{N}_{{{\rm{H}}}_{2}}({\mathrm{cm}}^{-2})﹩ in logarithmic scales. The values on the x-axis for these parameters correspond to the bin values from the second to the end value, while ﹩\mathrm{log}{N}_{{{\rm{H}}}_{2}}﹩ shows bin values on the top x-axis from the second to the end. The bin values and detection rates are presented in Table 5.

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