We 21 - A WN 8 star in a planetary nebula

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Photometry, Emission Spectra, Planetary Nebulae, Wolf-Rayet Stars, Forbidden Transitions, Oxygen Spectra, Stellar Magnitude, Stellar Mass Ejection, Ubv Spectra

Scientific paper

Direct imaging, photometry, and optical and mm-spectroscopy of We 21
shows that this object is a subluminous WN 8 star with an absolute
magnitude near Mv = -1.3. It is the central star of a low-excitation,
possibly nitrogen-rich planetary nebula, which interacts with dense
interstellar material of the inner Carina arm.

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