Abstract
An unusual face-on spiral in the wind of the M-type AGB star EP Aquarii <i>(Corrigendum)</i>
Highlights
It has been brought to our attention that an error was made in the measurement of the continuum flux density
1.33 Jy, while it is only 1.86 mJy. This implies that the deduction of the total dust mass that resides within this region (∼5 × 10−6 M ) was false
We cannot correct this estimate by performing the same analysis to the updated flux measurement because our estimate of the stellar continuum flux contribution of 2.27 × 10−2 Jy exceeds the updated value
Summary
It has been brought to our attention that an error was made in the measurement of the continuum flux density 2 JBCA, Department Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK 3 School of Chemistry, University of Leeds, Leeds LS2 9JT, UK 4 LESIA (CNRS UMR 8109), Observatoire de Paris, PSL, CNRS, UPMC, Univ.
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