Wind fluctuations observed for the [WC9] nucleus of the planetary nebula BD+30 3639.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Planetary Nebulae: Central Stars, Stars: Wolf-Rayet, Stellar Winds

Scientific paper

The CIII and CIV lines in the [WC9] spectrum of BD+30 3639 show variable
features, interpreted in terms of radiative acceleration of "blobs"
forming in the wind. The variations are like those observed for the WC9
massive stars, and the blobs acceleration appears smaller than for the
[WC8] nucleus of NGC 40.

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