Multitechnique testing of the viscous decretion disk model (Corrigendum)

R. Klement; A. C. Carciofi; Th. Rivinius; D. Panoglou; R. G. Vieira; J. E. Bjorkman; S. Štefl; C. Tycner; D. M. Faes; D. Korčáková; A. Müller; R. T. Zavala; M. Curé

doi:10.1051/0004-6361/201526535e

Free Access

Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 607, November 2017


Article Number		C1
Number of page(s)		1
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201526535e
Published online		10 November 2017

A&A 607, C1 (2017)

I. The stable and tenuous disk of the late-type Be star β CMi

R. Klement¹, A. C. Carciofi², Th. Rivinius³, D. Panoglou², R. G. Vieira², J. E. Bjorkman⁴, S. Štefl^†, C. Tycner⁵, D. M. Faes², D. Korčáková¹, A. Müller³, R. T. Zavala⁶ and M. Curé⁷

¹ Astronomical Institute of Charles University, Charles University in Prague, V Holešovičkách 2, 180 00 Prague 8, Czech Republic
e-mail: robertklement@gmail.com
² Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão 1226, Cidade Universitária, 05508-900 São Paulo, SP, Brazil
³ European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19, Chile
⁴ Ritter Observatory, Department of Physics & Astronomy, University of Toledo, Toledo, OH 43606, USA
⁵ Department of Physics, Central Michigan University, Mount Pleasant, MI 48859, USA
⁶ US Naval Observatory, Flagstaff Station, 10391 W. Naval Observatory Rd., Flagstaff, AZ 86001, USA
⁷ Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Casilla 5030, Valparaíso, Chile

This article has no abstract.

Key words: stars: emission-line, Be / stars: individual: βCMi / radio continuum: stars / submillimeter: stars / techniques: polarimetric / errata, addenda

^†

Deceased.

Erratum to: A&A 584, A85 (2015), DOI: 10.1051/0004-6361/201526535

© ESO, 2017

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