ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE
The discrepancy between the photometric and spectroscopic mass-ratio in W UMa-type systems is examined by using all the available mass-ratio data derived by modern techniques from photoelectric and radial velocity curves. The new additional data confirm, with few exceptions, the dependence of the di...
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Format: | Article |
Language: | English |
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Odessa I. I. Mechnykov National University
2017-06-01
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Series: | Odessa Astronomical Publications |
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Online Access: | http://oap.onu.edu.ua/article/view/103640 |
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author | P. G. Niarchos H. W. Dnerbeck |
author_facet | P. G. Niarchos H. W. Dnerbeck |
author_sort | P. G. Niarchos |
collection | DOAJ |
description | The discrepancy between the photometric and spectroscopic mass-ratio in W UMa-type systems is examined by using all the available mass-ratio data derived by modern techniques from photoelectric and radial velocity curves. The new additional data confirm, with few exceptions, the dependence of the discrepancy on the spectral type, first established by Niarchos and Duerbeck (1991). It is suggested that this discrepancy may be due to the influence of a global circulation pattern on the measured radial velocities. |
first_indexed | 2024-12-14T22:49:47Z |
format | Article |
id | doaj.art-4a1b82f462d14646a7c3fe3403310a9b |
institution | Directory Open Access Journal |
issn | 1810-4215 |
language | English |
last_indexed | 2024-12-14T22:49:47Z |
publishDate | 2017-06-01 |
publisher | Odessa I. I. Mechnykov National University |
record_format | Article |
series | Odessa Astronomical Publications |
spelling | doaj.art-4a1b82f462d14646a7c3fe3403310a9b2022-12-21T22:44:45ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-06-01100374010.18524/1810-4215.1997.10.103640103640ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPEP. G. Niarchos0H. W. Dnerbeck1Section of Astrophysics, Astronomy and Mechanics Department of Physics, University of AthensAstronomy Department Universidad Catoiica del NorteThe discrepancy between the photometric and spectroscopic mass-ratio in W UMa-type systems is examined by using all the available mass-ratio data derived by modern techniques from photoelectric and radial velocity curves. The new additional data confirm, with few exceptions, the dependence of the discrepancy on the spectral type, first established by Niarchos and Duerbeck (1991). It is suggested that this discrepancy may be due to the influence of a global circulation pattern on the measured radial velocities.http://oap.onu.edu.ua/article/view/103640binarieseclipsingstars massratiostars: w uma systems |
spellingShingle | P. G. Niarchos H. W. Dnerbeck ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE Odessa Astronomical Publications binaries eclipsing stars massratio stars: w uma systems |
title | ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE |
title_full | ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE |
title_fullStr | ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE |
title_full_unstemmed | ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE |
title_short | ON THE MASS-RATIO OF THE ECLIPSING BINARIES OF W UMa TYPE |
title_sort | on the mass ratio of the eclipsing binaries of w uma type |
topic | binaries eclipsing stars massratio stars: w uma systems |
url | http://oap.onu.edu.ua/article/view/103640 |
work_keys_str_mv | AT pgniarchos onthemassratiooftheeclipsingbinariesofwumatype AT hwdnerbeck onthemassratiooftheeclipsingbinariesofwumatype |