Issue |
A&A
Volume 639, July 2020
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 3 | |
Section | Catalogs and data | |
DOI | https://doi.org/10.1051/0004-6361/201935359e | |
Published online | 03 July 2020 |
MONOS: Multiplicity Of Northern O-type Spectroscopic systems
I. Project description and spectral classifications and visual multiplicity of previously known objects (Corrigendum)
1
Centro de Astrobiología, CSIC-INTA. Campus ESAC, Camino bajo del castillo s/n, 28 692 Vill. de la Cañada, Madrid, Spain
e-mail: jmaiz@cab.inta-csic.es
2
Departamento de Física Aplicada. Universidad de Alicante, Ctra. S. Vicente del Raspeig, 03 690 S. Vicente del Raspeig, Spain
3
Departamento de Física y Astronomía. Universidad de La Serena, Av. cisternas 1200 norte, La Serena, Chile
4
Instituto de Astrofísica de Canarias, 38 200 La Laguna, Tenerife, Spain
5
Departamento de Astrofísica. Universidad de La Laguna, 38 205 La Laguna, Tenerife, Spain
6
Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la astronomía s/n, 18 008 Granada, Spain
7
Instituto de Astrofísica de La Plata (CONICET, UNLP), Paseo del bosque s/n, 1900 La Plata, Argentina
8
Isaac Newton Group of Telescopes, Apartado de correos 321, 38 700 Santa Cruz de La Palma, La Palma, Spain
9
Agrupación Astronómica de Huesca, Parque Tecnológico Walqa, parcela 13, 22 197 Huesca, Spain
10
Las Campanas Observatory. Carnegie Observatories, Casilla 601, La Serena, Chile
11
Department of Physics and Astronomy, State University of New York at Geneseo, 1 College Circle, Geneseo, NY 14 454, USA
12
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Ctra. S. Vicente del Raspeig, 03 690 S. Vicente del Raspeig, Spain
Key words: stars: kinematics and dynamics / stars: early-type / binaries: general / errata, addenda
An inconsistency in the header information of some AstraLux files was detected after the publication of the paper. As a result, the heliocentric Julian date (HJD) of some of the observations was incorrectly listed in Table A.1. The error was half a day at most and it only affects systems with long periods, so the difference is irrelevant for any orbit calculation given the uncertainties involved. Nevertheless, we provide an updated version of Table A.1 with the appropriate corrections.
Appendix A: Additional figures and tables
Measurements for visual pairs using our AstraLux lucky images.
© ESO 2020
All Tables
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