ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz

L. Decin; A. M. S. Richards; T. Danilovich; W. Homan; J. A. Nuth

doi:10.1051/0004-6361/201732216e

Free Access

Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 621, January 2019


Article Number		C2
Number of page(s)		6
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201732216e
Published online		07 January 2019

A&A 621, C2 (2019)

Corrigendum

ALMA spectral line and imaging survey of a low and a high mass-loss rate AGB star between 335 and 362 GHz

L. Decin¹, A. M. S. Richards², T. Danilovich¹, W. Homan¹ and J. A. Nuth³

¹ Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
e-mail: Leen.Decin@kuleuven.be
² JBCA, Department Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK
³ NASA/GSFC, Mail Code 690, Greenbelt, MD 20771, USA

Key words: stars: AGB and post-AGB / stars: mass-loss / circumstellar matter / stars: individual: IK Tau / stars: individual: R Dor / errata, addenda

Erratum to: A&A, 615, A28 (2018), https://doi.org/10.1051/0004-6361/201732216

An error occurred in Table A.2 during the production process: some extra values have been inserted. Here we publish the correct Table A.2.

© ESO 2019

All Tables

Table A.2.

Spectral lines observed in R Dor with ALMA.

In the text

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