Figure 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 1 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 2 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 3 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 4 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 5 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 6 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 7 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 8 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 9 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 10 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 11 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 12 of 12) Yoshimasa Watanabe et al. 2015 ApJ 809 162 doi:10.1088/0004-637X/809/2/162 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.