Figure 1 from The First “Water Fountain” Collimated Outflow in a Planetary Nebula

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The First “Water Fountain” Collimated Outflow in a Planetary Nebula

Authors: José F. Gómez, Olga Suárez, Philippe Bendjoya, J. Ricardo Rizzo, Luis F. Miranda, James A. Green, Lucero Uscanga, Enrique García-García, Eric Lagadec, Martín A. Guerrero, and Gerardo Ramos-Larios

Gómez et al. 2015 The Astrophysical Journal 799 186.

Provider: AAS Journals

Caption: Figure 1.

Water maser spectra toward I15103, in two different epochs, integrating over the whole emitting region. The component with the highest flux density (1.731 kJy) in the left panel has been truncated, so that weaker components can be seen.

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