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Cited article:

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The GW Vir Instability Strip in Light of New Observations of PG 1159 Stars: Discovery of Pulsations in the Central Star of A72 and Variability of RX J0122.9–7521

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Relativistic atomic structure calculations and evaluation of plasma parameters in Be-like ions for its possible use in laboratory plasma diagnostic studies

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Search for trans-iron elements in hot, helium-rich white dwarfs with the HST Cosmic Origins Spectrograph

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Benchmarking Atomic Data for Astrophysics: Be-like Ions between B ii and Ne vii

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SYSTEMATIC CALCULATIONS OF ENERGY LEVELS AND TRANSITION RATES OF BE-LIKE IONS WITH Z = 10–30 USING A COMBINED CONFIGURATION INTERACTION AND MANY-BODY PERTURBATION THEORY APPROACH

K. Wang, X. L. Guo, H. T. Liu, et al.
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Analysis of HST/COS spectra of the bare C–O stellar core H1504+65 and a high-velocity twin in the Galactic halo

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FTIR laboratory measurement of Ne i Rydberg states in 1.43−14.3μm spectral range

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Astronomy & Astrophysics 582 A12 (2015)
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UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3

Graziela R. Keller, Luciana Bianchi and Walter J. Maciel
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Raman-scattered Ne vii λ973 at 4881 Å in the symbiotic star V1016 Cygni

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Monthly Notices of the Royal Astronomical Society 442 (3) 1956 (2014)
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Weak metal lines in optical high-resolution Very Large Telescope and Keck spectra of “cool” PG 1159 stars

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Analysis of far-UV data of central stars of planetary nebulae: Occurrence and variability of stellar winds

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New advances in the field of planetary nebulae from ultraviolet observations

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Iron abundance in the prototype PG 1159 star, GW Vir pulsator PG 1159 − 035, and related objects

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Astronomy & Astrophysics 531 A146 (2011)
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AGB star intershell abundances inferred from UV spectra of extremely hot post-AGB stars

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The metallicity extremes of the Sagittarius dSph: SALT spectroscopy of PNe★

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NeiiStark Width and Shift Regularities

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The Astrophysical Journal 687 (2) 1423 (2008)
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Non-LTE Spectral Analysis of Extremely Hot Post-AGB Stars: Constraints for Evolutionary Theory

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Identification of Ne VIII lines in H-deficient (pre-) white dwarfs: a new tool to constrain the temperature of the hottest stars

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Discovery of photospheric argon in very hot central stars of planetary nebulae and white dwarfs

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CHIANTI—An Atomic Database for Emission Lines. VII. New Data for X‐Rays and Other Improvements

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The Elemental Abundances in Bare Planetary Nebula Central Stars and the Shell Burning in AGB Stars

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Structure and Evolution of White Dwarfs and their Interaction with the Local Interstellar Medium

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Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories

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Fundamental Questions in Astrophysics: Guidelines for Future UV Observatories 3 (2006)
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The mass of helium in white dwarf stars and the formation and evolution of hydrogen-deficient post-AGB stars

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Ab initiocalculations with CI+MBPT of large number of energy levels for beryllium-like neon

I M Savukov and A A Markhotok
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Discovery of Neviiin the Winds of Hot Evolved Stars

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The Astrophysical Journal 627 (1) 424 (2005)
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Abundance of Elements beyond the Iron Group in Cool DO White Dwarfs

P. Chayer, S. Vennes, J. Dupuis and J. W. Kruk
The Astrophysical Journal 630 (2) L169 (2005)
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