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Pillars of Creation among Destruction: Star Formation in Molecular Clouds near R136 in 30 Doradus

  • Authors: Venu M. Kalari, Mónica Rubio, Bruce G. Elmegreen, Viviana V. Guzmán, Hans Zinnecker, and Cinthya N. Herrera

2018 The Astrophysical Journal 852 71.

  • Provider: AAS Journals

Caption: Figure 5.

(a) The peak velocity in the frame of the local standard of rest (﹩{V}_{\mathrm{lsr}}﹩) of each cloud is plotted as a function of projected distance from R136. The upper y-axis gives the projected distance in arcmin, while the lower y-axis gives it in parsecs assuming a distance of 50 kpc. The best-fit relation is given by the dashed line and has a slope of ∼1.5. (b) The mass of each cloud ﹩{M}_{{{\rm{H}}}_{2}}﹩ is plotted as a function of projected distance from R136. The upper y-axis gives the projected distance in arcmin, while the lower y-axis gives it in parsecs assuming a distance of 50 kpc. The best-fit relation is given by the dashed line.

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