Artículo . Monthly Notices of the Royal Astronomical Society ; vol. 433, nº 2

Apsidal motion in massive close binary systems

I. HD 165052 an extreme case?

Ferrero, G. | Gamen, R. | Benvenuto, Omar Gustavo | Fernández Lajús, E.
Abstract: We present a new set of radial-velocity measurements of the spectroscopic binary HD 165052 obtained by disentangling of high-resolution optical spectra. The longitude of the periastron (̟ $latex \varpi $, which was used to calculate the absolute masses of the binary components: M1 = 22.
Abstract: We present a new set of radial-velocity measurements of the spectroscopic binary HD 165052 obtained by disentangling of high-resolution optical spectra. The longitude of the periastron (̟ $latex \varpi $, which was used to calculate the absolute masses of the binary components: M1 = 22.5 ± 1.0 M⊙ and M2 = 20.5 ± 0.9 M⊙. Analysing the separated spectra we have re-classified the components as O7Vz and O7.5Vz stars.
  • Origin info: Universidad Nacional de La Plata
  • Subject: Astronomía
  • Lenguage: Inglés
  • Extension: 14 p.

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  • Date of availability: 12 de septiembre de 2016
  • Date of accession: 12 de septiembre de 2016
  • Date issued: 2013
  • Others identifiers: DOI:10.1093/mnras/stt812
  • URL to resource: https://digital.cic.gba.gob.ar/handle/11746/4212
  • Licence: Attribution 4.0 International (BY 4.0)
http://creativecommons.org/licenses/by/4.0/
This work is published under license Creative Commons Attribution 4.0 International (BY 4.0)
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