| Issue |
A&A
Volume 588, April 2016
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201321819e | |
| Published online | 25 March 2016 | |
Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry (Corrigendum)
1 European Southern Observatory, Karl-Schwarzschild Straße 2, 85748 Garching bei München, Germany
e-mail: nkains@eso.org
2 Instituto de Astronomía, Universidad Nacional Autónoma de Mexico 0410 Ciudad de México, Mexique
3 SUPA School of Physics & Astronomy, University of St. Andrews, North Haugh, St. Andrews, KY16 9SS, UK
4 Niels Bohr Institute, University of Copenhagen, Juliane Maries vej 30, 2100 Copenhagen, Denmark
5 Centre for Star and Planet Formation, Geological Museum, Øster Voldgade 5, 1350 Copenhagen, Denmark
6 Indian Institute of Astrophysics, 560034 Koramangala, Bangalore, India
7 Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA
8 Qatar Foundation, PO Box 5825, Doha, Qatar
9 Department of Astronomy, Boston University, 725 Commonwealth Ave, Boston, MA 02215, USA
10 Dipartimento di Fisica “E.R Caianiello”, Universitá di Salerno, via Ponte Don Melillo, 84084 Fisciano, Italy
11 Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, 80100 Napoli, Italy
12 HE Space Operations GmbH, Flughafenallee 24, 28199 Bremen, Germany
13 Istituto Internazionale per gli Alti Studi Scientifici (IIASS), 84019 Vietri Sul Mare (SA), Italy
14 Institut d’Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 17, Sart Tilman, Bât. B5c, 4000 Liège, Belgium
15 Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg (ZAH), Mönchhofstr. 12−14, 69120 Heidelberg, Germany
16 Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
17 Main Astronomical Observatory, Academy of Sciences of Ukraine, vul. Akademika Zabolotnoho 27, 03680 Kyiv, Ukraine
18 National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, 650011 Kunming, PR China
19 Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, PR China
20 Korea Astronomy and Space Science Institute, 305-348 Daejeon, Korea
21 Institut for Rumforskning og -teknologi, Danmarks Tekniske Universitet, 2800 København, Denmark
22 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, 8000 Aarhus C, Denmark
23 Jodrell Bank Centre for Astrophysics, University of Manchester, Oxford Road, Manchester, M13 9PL, UK
24 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
25 Perth Observatory, Walnut Road, Bickley, 6076 Perth, Australia
26 Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, 7820436 Macul, Santiago, Chile
27 Department of Physics, Sharif University of Technology, PO Box 4, 11155–9161 Tehran, Iran
28 Perimeter Institute for Theoretical Physics, 31 Caroline St. N., Waterloo ON, N2L 2Y5, Canada
29 Instituto de Astronomía – UNAM, Km 103 Carretera Tijuana Ensenada, 422860 Ensenada (Baja Cfa), Mexico
30 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
31 INFN, Gruppo Collegato di Salerno, Sezione di Napoli, Italy
32 Max Planck Institute for Solar System Research,Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
33 Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
Key words: stars: variables: general / stars: variables: RR Lyrae / globular clusters: individual: M 30 (NGC 7099) / errata, addenda
The paper “Estimating the parameters of globular cluster M 30 (NGC 7099) from time-series photometry”, used an incorrect expression for the phase φ(t) at time t of a periodic variable undergoing a linear period change. Equation (3) of that paper should be: 
(1)where NE(t) is the number of cycles elapsed at time t since a reference epoch E. For a constant rate of period change β, NE(t) is given by (Kains et al. 2015): ![\begin{equation} N_{E}(t) = \frac{1}{\beta} \ln \left[1 + \frac{\beta}{P_{0}} (t - E) \right] , \end{equation}](/articles/aa/full_html/2016/04/aa21819e-13/aa21819e-13-eq8.png)
(2)where P0 is the period at the epoch E. Using this correct expression, we are still unable to phase the light curve of RR Lyrae star V16 satisfactorily, and our conclusions therefore remain unaffected.
References
- Kains, N., Arellano Ferro, A., Figuera Jaimes, R., et al. 2015, A&A, 578, A128 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2016
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.