| Issue |
A&A
Volume 593, September 2016
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201526027e | |
| Published online | 01 September 2016 | |
A remarkable recurrent nova in M31: Discovery and optical/UV observations of the predicted 2014 eruption (Corrigendum)
1 Astrophysics Research Institute,
Liverpool John Moores University, IC2
Liverpool Science Park Liverpool, L3
5RF, UK
e-mail: M.J.Darnley@ljmu.ac.uk
2 Institut de Ciències de l’Espai
(CSIC-IEEC), Campus UAB, C/Can
Magrans s/n, 08193
Cerdanyola del Valles,
Spain
3 Department of Astrophysics/IMAPP,
Radboud University, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
4 Instituto de Astrofísica de Canarias,
Vía Láctea, s/n, La
Laguna, 38205
Santa Cruz de Tenerife,
Spain
5 Departamento de Astrofísica,
Universidad de La Laguna, La
Laguna, 38206
Santa Cruz de Tenerife,
Spain
6 Department of Astronomy, San Diego
State University, San
Diego, CA
92182,
USA
7 Physics Department, Lancaster
University, Lancaster, LA1
4YB, UK
8 Department of Earth Science and
Astronomy, College of Arts and Sciences, The University of Tokyo,
3-8-1 Komaba, Meguro-ku, 153-8902
Tokyo,
Japan
9 Astronomical Institute, Academy of
Sciences, 251 65
Ondřejov, Czech
Republic
10 Astronomy Department, University of
Illinois at Urbana-Champaign, 1002
W. Green Street, Urbana, IL
61801,
USA
11 Department of Astronomy, Keio
University, Hiyoshi,
223-8521
Yokohama,
Japan
12 Variable Stars Observers League in
Japan (VSOLJ), 7-1 Kitahatsutomi, 273-0126 Kamagaya,
Japan
13 Astronomical Institute of the Charles University, Faculty
of Mathemathics and Physics, V Holešovičkách 2, 180 00 Praha 8, Czech Republic
14 Okayama Astrophysical Observatory,
NAOJ, NINS, 3037-5 Honjo, Kamogata,
Asakuchi, 719-0232
Okayama,
Japan
15 European Space Astronomy Centre,
Camino Bajo del Castillo s/n, Urb. Villafranca del Castillo, 28692 Villanueva de la
Cañada, Madrid,
Spain
16 Departament de Física i Enginyeria
Nuclear, EUETIB, Universitat Politècnica de Catalunya, c/ Compte d’Urgell 187, 08036
Barcelona,
Spain
17 Institut d’Estudis Espacials de
Catalunya, c/ Gran Capità 2-4, Ed.
Nexus-201, 08034
Barcelona,
Spain
18 Isaac Newton Group of Telescopes,
Apartado de correos 321, 38700
Santa Cruz de La Palma,
Spain
Key words: galaxies: individual: M31 / novae, cataclysmic variables / stars: individual: M31N 2008-12a / errata, addenda
An error has been identified in Table 3 of Darnley et al. (2015). The original table of fluxes included the incorrect unit (× 10-15 W m-2). The correct unit should have been (× 10-15 erg cm-2 s-1), and hence a discrepancy of a factor of 1000 was introduced.
No other parts of the paper, nor the results reported within, were affected by this error. We have included a corrected version in Table 1.
Selected observed emission lines and fluxes from the three epochs of Liverpool Telescope SPRAT spectra of the 2014 eruption of M31N 2008-12a.
References
- Darnley, M. J., Henze, M., Steele, I. A., et al. 2015, A&A, 580, A45 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO 2016
All Tables
Selected observed emission lines and fluxes from the three epochs of Liverpool Telescope SPRAT spectra of the 2014 eruption of M31N 2008-12a.
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