Orbital and physical properties of the s Ori Aa, Ab, B triple system


Por: Simón-Díaz S., Caballero J.A., Lorenzo J., Maíz Apellániz J., Schneider F.R.N., Negueruela I., Barbá R.H., Dorda R., Marco A., Montes D., Pellerin A., Sanchez-Bermudez J., Sódor Á., Sota A.

Publicada: 1 ene 2015
Resumen:
We provide a complete characterization of the astrophysical properties of the s Ori Aa, Ab, B hierarchical triple system and an improved set of orbital parameters for the highly eccentric s Ori Aa, Ab spectroscopic binary. We compiled a spectroscopic data set comprising 90 high-resolution spectra covering a total time span of 1963 days. We applied the Lehman-Filhés method for a detailed orbital analysis of the radial velocity curves and performed a combined quantitative spectroscopic analysis of the s Ori Aa, Ab, B system by means of the stellar atmosphere code fastwind. We used our own plus other available information on photometry and distance to the system for measuring the radii, luminosities, and spectroscopic masses of the three components.We also inferred evolutionary masses and stellar ages using the Bayesian code bonnsai. The orbital analysis of the new radial velocity curves led to a very accurate orbital solution of the s Ori Aa, Ab pair.We provided indirect arguments indicating that s Ori B is a fast-rotating early B dwarf. The FASTWIND+BONNSAI analysis showed that the Aa, Ab pair contains the hottest and most massive components of the triple system while s Ori B is a bit cooler and less massive. The derived stellar ages of the inner pair are intriguingly younger than the one widely accepted for the s Orionis cluster, at 3 ± 1 Ma. The outcome of this study will be of key importance for a precise determination of the distance to the s Orionis cluster, the interpretation of the strong X-ray emission detected for s Ori Aa, Ab, B, and the investigation of the formation and evolution of multiple massive stellar systems and substellar objects. © 2015. The American Astronomical Society. All rights reserved.

Filiaciones:
Simón-Díaz S.:
 Instituto de Astrofisica de Canarias, La Laguna, Tenerife, E-38200, Spain

 Departamento de Astrofísica, Universidad de la Laguna, La Laguna, Tenerife, E-38205, Spain

Caballero J.A.:
 Centro de Astrobiología (CSIC-INTA), ESAC Campus, P.O. Box 78, Villanueva de la Cañada, Madrid, E-28691, Spain

Lorenzo J.:
 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Escuela Politécnica Superior, University of Alicante, Apdo. 99, Alicante, E-03080, Spain

Maíz Apellániz J.:
 Centro de Astrobiología (CSIC-INTA), ESAC Campus, P.O. Box 78, Villanueva de la Cañada, Madrid, E-28691, Spain

 Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, Granada, E-18008, Spain

Schneider F.R.N.:
 Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, Bonn, D-53121, Germany

Negueruela I.:
 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Escuela Politécnica Superior, University of Alicante, Apdo. 99, Alicante, E-03080, Spain

Barbá R.H.:
 Departamento de Física, Universidad de La Serena, Benavente 980, La Serena, Chile

Dorda R.:
 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Escuela Politécnica Superior, University of Alicante, Apdo. 99, Alicante, E-03080, Spain

Marco A.:
 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Escuela Politécnica Superior, University of Alicante, Apdo. 99, Alicante, E-03080, Spain

Montes D.:
 Departamento Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Madrid, E-28040, Spain

Pellerin A.:
 Department of Physics and Astronomy, State University of New York at Geneseo, 1 College Circle, Geneseo, NY 14454, United States

Sanchez-Bermudez J.:
 Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, Granada, E-18008, Spain

Sódor Á.:
 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, Budapest, H-01121, Hungary

Sota A.:
 Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la Astronomía s/n, Granada, E-18008, Spain
ISSN: 0004637X
Editorial
UNIV CHICAGO PRESS, 1427 E 60TH ST, CHICAGO, IL 60637-2954 USA, Estados Unidos America
Tipo de documento: Article
Volumen: 799 Número: 2
Páginas:
WOS Id: 000348820900056
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