Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been obtained combining échelle and coudé CCD observations. The radial velocity orbits derived from the He iiλ4686 Å (primary component) and He iλ4471 Å (secondary component) absorption lines yield semi-amp...
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Autores principales: | , , , , , , , , , , |
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Formato: | Articulo |
Lenguaje: | Inglés |
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2001
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2072 http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2001.04500.x/pdf http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2001.04500.x/full |
Aporte de: |
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I19-R120-10915-2072 |
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record_format |
dspace |
institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Astronómicas Astrofísica binaries: general stars: early-type stars: individual: HD 93205 X-rays: stars |
spellingShingle |
Ciencias Astronómicas Astrofísica binaries: general stars: early-type stars: individual: HD 93205 X-rays: stars Morrell, Nidia Irene Barbá, Rodolfo Héctor Niemelä, Virpi Sinikka Corti, Mariela Alejandra Albacete Colombo, Juan Facundo Rauw, G. Corcoran, Michael Morel, T. Bertrand, J. F. Moffat, Anthony St-Louis, Nicole Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
topic_facet |
Ciencias Astronómicas Astrofísica binaries: general stars: early-type stars: individual: HD 93205 X-rays: stars |
description |
A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been obtained combining échelle and coudé CCD observations. The radial velocity orbits derived from the He iiλ4686 Å (primary component) and He iλ4471 Å (secondary component) absorption lines yield semi-amplitudes of 133±2 and 314±2 km s−1 for each binary component, resulting in minimum masses of 31 and 13 M⊙(q=0.42). We also confirm for the binary components the spectral classification of O3 V+ O8 V previously assigned. Assuming for the O8 V component a ‘normal’ mass of 22–25 M⊙ we would derive for the primary O3 V a mass of ‘only’52–60 M⊙ and an inclination of about 55° for the orbital plane. We have also determined for the first time a period of apsidal motion for this system, namely 185±16 yr using all available radial velocity data sets of HD 93205 (from 1975 to 1999). Phase-locked variations of the X-ray emission of HD 93205 consisting of a rise of the observed X-ray flux near periastron passage are also discussed. |
format |
Articulo Articulo |
author |
Morrell, Nidia Irene Barbá, Rodolfo Héctor Niemelä, Virpi Sinikka Corti, Mariela Alejandra Albacete Colombo, Juan Facundo Rauw, G. Corcoran, Michael Morel, T. Bertrand, J. F. Moffat, Anthony St-Louis, Nicole |
author_facet |
Morrell, Nidia Irene Barbá, Rodolfo Héctor Niemelä, Virpi Sinikka Corti, Mariela Alejandra Albacete Colombo, Juan Facundo Rauw, G. Corcoran, Michael Morel, T. Bertrand, J. F. Moffat, Anthony St-Louis, Nicole |
author_sort |
Morrell, Nidia Irene |
title |
Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
title_short |
Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
title_full |
Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
title_fullStr |
Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
title_full_unstemmed |
Optical spectroscopy of X-Mega targets : II. The massive double-lined O-type binary HD93205 |
title_sort |
optical spectroscopy of x-mega targets : ii. the massive double-lined o-type binary hd93205 |
publishDate |
2001 |
url |
http://sedici.unlp.edu.ar/handle/10915/2072 http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2001.04500.x/pdf http://onlinelibrary.wiley.com/doi/10.1046/j.1365-8711.2001.04500.x/full |
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