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Context. There are more than 3000 true and probable known Galactic Planetary Nebulae (PNe), but only for 13% of them there is central star spectroscopic information available. Aims. To contribute to t...
Over the past decade, the number of planetary nebula central stars (CSPN) known to exhibit the Wolf-Rayet (WR) phenomenon has grown substantially. Many of these discoveries have resulted from the Macq...
A number of efforts are underway to detect close binary stars in planetary nebulae. The primary goal of these studies is to determine the binary fraction of central stars.
The low excitation planetary nebulae HuDo1 and HuBi1 and their [WC10] central stars
A Dynamical Model for PNE with WR-Type Central Stars
Expansion Velocities of Planetary Nebulae with [WC] Central Stars
Of Wolf-Rayet Central Stars and Common Envelopes
Expansion velocities from different ions of planetary nebulae with [wc]-type central stars
Physical properties of Planetary nebulae around [WC] central stars
Characteristics of Planetary Nebulae with [WC] Central Stars

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