The common envelope origins of the fast jet in the planetary nebula M 3-38

Abstract

We present the analysis of Multi-Espectrógrafo en GTC de Alta Resolución para Astronomía (MEGARA) high-dispersion integral field spectroscopic observations of the bipolar planetary nebula (PN) M 3-38. These observations unveil the presence of a fast outflow aligned with the symmetry axis of M 3-38 that expands with a velocity up to $\pm$225 km s${}^{-1}$. The deprojected space velocity of this feature can be estimated to be $\approx$320${}_{-60}^{+130}$ km s${}^{-1}$, which together with its highly collimated morphology suggests that it is one of the fastest jet detected in a PN. We have also used Kepler observations of the central star of M 3-38 to unveil variability associated with a dominant period of 17.7 days. We attribute this to the presence of a low-mass star with an orbital separation of $\approx$0.12-0.16 au. The fast and collimated ejection and the close binary system point towards a common envelope formation scenario for M 3-38.

9 pages, 5 figures, Accepted ApJ Letter

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• The origin of the planetary nebula M 1-16. A morphokinematic and chemical analysis
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