First image of the circumstellar envelope of the red supergiant MU CEP in the NA I 5890 A line

Astronomy and Astrophysics – Astrophysics

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Cepheid Variables, Emission Spectra, Red Giant Stars, Semiregular Variable Stars, Sodium Compounds, Stellar Envelopes, Supergiant Stars, Fabry-Perot Interferometers, M Stars, Stellar Composition, Stellar Evolution, Stellar Structure, Stellar Winds

Scientific paper

The first image (actually interferogram) of the circumstellar envelope of the luminous red supergiant μ Cep has been obtained by Fabry-Pérot interferometry in the Na I λ5890 Å line. No K I scattering was detected. The Na I emission is found up to about 30 arcseconds from the star, an extension possibly related with the stellar lifetime in the red giant phase. The envelope appears strongly asymmetric and inhomogeneous. Although dynamical interaction with the interstellar medium is not ruled out, the observations strengthen the case of an episodic and not spherically symmetric wind, agreeing with the presence of multiple circumstellar components in the stellar spectra.

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