Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass.

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Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 1 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 2 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 3 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 4 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 5 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 6 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 7 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

Figure 14 from MUSCLE W49: A Multi-Scale Continuum and Line Exploration of the Most Luminous Star Formation Region in the Milky Way. I. Data and the Mass Structure of the Giant Molecular Cloud (Image 8 of 8) R. Galván-Madrid et al ApJ doi: / X/779/2/121 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.