Figure 6 from A Detailed Study of the Structure of the Nested Planetary Nebula, Hb 12, the Matryoshka Nebula

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A Detailed Study of the Structure of the Nested Planetary Nebula, Hb 12, the Matryoshka Nebula

Authors: D. M. Clark, J. A. López, M. L. Edwards, and C. Winge

Clark et al. 2014 The Astronomical Journal 148 98.

Provider: AAS Journals

Caption: Figure 6.

Brγ line emission from the nuclear region presented in a long-slit format. Blobs of emission on either side of the core, slightly displaced along the slit by 0 farcs 1 from each other and at ±45 km s⁻¹from the line center, are indicative of a bipolar flow emerging very close to the nucleus. Fainter emission reaches ±90 km s⁻¹.

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