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Cited article:

THE DOUBLE-DEGENERATE NUCLEUS OF THE PLANETARY NEBULA TS 01: A CLOSE BINARY EVOLUTION SHOWCASE

Gagik Tovmassian, Lev Yungelson, Thomas Rauch, et al.
The Astrophysical Journal 714 (1) 178 (2010)
https://doi.org/10.1088/0004-637X/714/1/178

The chemical composition of TS 01, the most oxygen-deficient planetary nebula

G. Stasińska, C. Morisset, G. Tovmassian, et al.
Astronomy and Astrophysics 511 A44 (2010)
https://doi.org/10.1051/0004-6361/200912405

The most oxygen-poor planetary nebula: AGB nucleosynthesis at low metallicities

G. Stasińska, C. Morisset, G. Tovmassian, T. Rauch and T. Decressin
Proceedings of the International Astronomical Union 5 (S265) 94 (2009)
https://doi.org/10.1017/S1743921310000281

A Close Binary Nucleus in the Most Oxygen‐Poor Planetary Nebula PN G135.9+55.9

G. H. Tovmassian, R. Napiwotzki, M. G. Richer, et al.
The Astrophysical Journal 616 (1) 485 (2004)
https://doi.org/10.1086/424795

The kinematics of the most oxygen-poor planetary nebula PN G 135.9+55.9

M. G. Richer, J. A. López, W. Steffen, et al.
Astronomy & Astrophysics 410 (3) 911 (2003)
https://doi.org/10.1051/0004-6361:20031267

Observations of [S [CSC]iv[/CSC]] 10.5 μm and [N[CLC]e[/CLC] [CSC]ii[/CSC]] 12.8 μm in Two Halo Planetary Nebulae: Implications for Chemical Self-Enrichment

Harriet L. Dinerstein, Matthew J. Richter, John H. Lacy and K. Sellgren
The Astronomical Journal 125 (1) 265 (2003)
https://doi.org/10.1086/345572