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M 1–92 revisited: the chemistry of a common envelope nebula?
Published online by Cambridge University Press: 30 December 2019
Abstract
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We report on new molecular-line observations of the bipolar pre-planetary nebula M 1–92. The new IRAM 30 m MRT and NOEMA data shows the presence of shock induced chemistry in the nebula. From the derived [17O]/[18O] ratio, we suggest that the sudden mass loss event responsible for the formation of the nebula 1200 yr ago may also have resulted in the premature end of the AGB phase of the central star.
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- © International Astronomical Union 2019
References
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