Avison, A

Evans, A

Eyres, Stewart Paul shore

Gehrz, R D

Hajduk, M

Mohamed, S

Starrfield, S

Wagner, R M

Woodward, C E

Zijlstra, A

CLoK

ArticleErratum: ALMA reveals the aftermath of a white dwarf–brown dwarf merger in CK VulpeculaeEyres, Stewart Paul shore, Evans, A, Zijlstra, A, Avison, A, Gehrz, R D, Hajduk, M, Starrfield, S, Mohamed, S, Woodward, C E and Wagner, R MAvailable at http://clok.uclan.ac.uk/30489/Eyres, Stewart Paul shore, Evans, A, Zijlstra, A, Avison, A, Gehrz, R D, Hajduk, M, Starrfield, S, Mohamed, S, Woodward, C E et al (2019) Erratum: ALMA reveals the aftermath of a white dwarf–brown dwarf merger in CK Vulpeculae. Monthly Notices of the  Royal Astronomical Society . ISSN 1365-2966  It is advisable to refer to the publisher’s version if you intend to cite from the work.http://dx.doi.org/10.1093/mnras/stz2890For more information about UCLan’s research in this area go to http://www.uclan.ac.uk/researchgroups/ and search for <name of research Group>.For information about Research generally at UCLan please go to http://www.uclan.ac.uk/research/ All outputs in CLoK are protected by Intellectual Property Rights law, includingCopyright law.  Copyright, IPR and Moral Rights for the works on this site are retained by the individual authors and/or other copyright owners. Terms and conditions for use of this material are defined in the http://clok.uclan.ac.uk/policies/CLoKCentral Lancashire online Knowledgewww.clok.uclan.ac.ukErratum: ALMA reveals the aftermath of a whitedwarf–brown dwarf merger in CK VulpeculaeS. P. S. Eyres1,2, A. Evans3, A. Zijlstra4, A. Avison4, R. D. Gehrz5, M. Hajduk6,S. Starrfield7, S. Mohamed8, C. E. Woodward5, R. M. Wagner9,101Faculty of Computing, Engineering & Science, University of South Wales, Pontypridd CF37 1DL, UK2Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK3Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG, UK4Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, M13 9PL, UK5Minnesota Institute for Astrophysics, School of Physics & Astronomy, 116 Church Street SE, University of Minnesota,Minneapolis, MN 55455, USA6Space Radio-Diagnostics Research Centre, University of Warmia and Mazury, Prawochenskiego Str. 9, 10-720 Olsztyn, Poland7School of Earth and Space Exploration, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA8South African Astronomical Observatory, PO Box 9, Observatory 7935, Cape Town, Western Cape, South Africa9Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA10LBT Observatory, University of Arizona, Tucson, AZ 85721-0065, USAAccepted XXX. Received YYY; in original form 21st September 2019Key words: circumstellar matter – stars: individual, CK Vul – stars: peculiar – stars:jets – stars: winds, outflows – Submillimetre: stars – errata, addenda1 ERRATUMThis is an erratum for Eyres et al. (2018). In Figure 3(d) thedirection of the offset axis was reversed. The corrected Fig 1included in this erratum corrects this. No other changes arenecessary, and the direction of the position–velocity plot isnot a factor in any of the conclusions of the paper.REFERENCESEyres S. P. S., Evans A., Ziljstra, A., Avison, A., Gerhz R.D., Hajduck, M., Starrfield S. G., Mohamed, S., Wood-ward C. E., Wagner R. M., 2018, MNRAS, 481, 4931Downloaded from https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/stz2890/5603754 by University of Central Lancashire user on 07 November 2019(a) (c)(b) (d)3CH OH CNFigure 1. (a) Intensity map of CH3OH (colour scale, line 7 in Table 1 in the original paper); contours of dust continuum at 0.12 and0.48 mJy beam−1 for reference; (b) position–velocity plot along the dashed–line with arrow in (a); (c) intensity map of CN (colour scale,line 5 in Table 1 in the original paper), contours as (a); (d) position–velocity plot along the dashed–line with arrow in (b) from northto south. For the intensity maps in (a) and (c) the spatial resolution is represented by the small black circle to the bottom left in eachimage, where both the spectral line and continuum resolutions are over–plotted, but are indistinguishable at this scale.Downloaded from https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/stz2890/5603754 by University of Central Lancashire user on 07 November 2019

Erratum: ALMA reveals the aftermath of a white dwarf–brown dwarf merger in CK Vulpeculae

This is an erratum for Eyres et al. (2018). In fig. 3(d) the direction of the offset axis was reversed. The corrected Fig. 1 included in this erratum corrects this. No other changes are necessary, and the direction of the position-velocity plot is not a factor in any of the conclusions of the paper.</p

Eyres, S.~P.~S.

Evans, A.

Zijlstra, A.

Avison, A.

Gehrz, R.~D.

Hajduk, M.

Starrfield, S.

Mohamed, S.

Woodward, C.~E.

Wagner, R.~M.

The University of Manchester - Institutional Repository

Erratum: ALMA reveals the aftermath of a white dwarf-brown dwarf merger in CK Vulpeculae

http://clok.uclan.ac.uk/30489/1/30489%20stz2890.pdf

Erratum: ALMA reveals the aftermath of a white dwarf–brown dwarf merger in CK Vulpeculae

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