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Velocity (km/s)

Fig 15.16.

Spectrum of the 2.6 mm CO emission line from the core of the molecular cloud behind the Orion Nebula (Fig. 15.28.) The broad wings extend many tens of kilometers per second on both sides of the line center. [Jeffrey Mangum, NRAO/AUI/NSF]

Velocity (km/s)

Fig 15.15.

Cluster of masers in an expanding shell.

Fig 15.16.

Spectrum of the 2.6 mm CO emission line from the core of the molecular cloud behind the Orion Nebula (Fig. 15.28.) The broad wings extend many tens of kilometers per second on both sides of the line center. [Jeffrey Mangum, NRAO/AUI/NSF]

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