Thermal decoupling in W UMa binary systems

A study of thermal decoupling in short period near contact binaries is presented. Statistics of well-observed W UMa systems (now including data of EB-type light curve objects) characterize completely A- and W- type objects. W-type systems show a good linear correlation in the thermal decoupling vs....

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Autores principales: Lípari, Sebastián Luis, Sisteró, Roberto Félix
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1987
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/141512
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spelling I19-R120-10915-1415122024-04-26T13:50:18Z http://sedici.unlp.edu.ar/handle/10915/141512 Thermal decoupling in W UMa binary systems Lípari, Sebastián Luis Sisteró, Roberto Félix 1987 2022-09-05T14:19:49Z es Astronomía Galaxia A study of thermal decoupling in short period near contact binaries is presented. Statistics of well-observed W UMa systems (now including data of EB-type light curve objects) characterize completely A- and W- type objects. W-type systems show a good linear correlation in the thermal decoupling vs. spectral type diagram. The same correlation is valid for the lower border of the distribution of A-type systems, otherwise scattered in an area of large thermal decoupling. These empirical facts are discussed in terms of contact on near contact configurations. A complete version of this paper will be published in Publication Astronomical Soc. of the Pacific. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
spellingShingle Astronomía
Galaxia
Lípari, Sebastián Luis
Sisteró, Roberto Félix
Thermal decoupling in W UMa binary systems
topic_facet Astronomía
Galaxia
description A study of thermal decoupling in short period near contact binaries is presented. Statistics of well-observed W UMa systems (now including data of EB-type light curve objects) characterize completely A- and W- type objects. W-type systems show a good linear correlation in the thermal decoupling vs. spectral type diagram. The same correlation is valid for the lower border of the distribution of A-type systems, otherwise scattered in an area of large thermal decoupling. These empirical facts are discussed in terms of contact on near contact configurations. A complete version of this paper will be published in Publication Astronomical Soc. of the Pacific.
format Articulo
Comunicacion
author Lípari, Sebastián Luis
Sisteró, Roberto Félix
author_facet Lípari, Sebastián Luis
Sisteró, Roberto Félix
author_sort Lípari, Sebastián Luis
title Thermal decoupling in W UMa binary systems
title_short Thermal decoupling in W UMa binary systems
title_full Thermal decoupling in W UMa binary systems
title_fullStr Thermal decoupling in W UMa binary systems
title_full_unstemmed Thermal decoupling in W UMa binary systems
title_sort thermal decoupling in w uma binary systems
publishDate 1987
url http://sedici.unlp.edu.ar/handle/10915/141512
work_keys_str_mv AT liparisebastianluis thermaldecouplinginwumabinarysystems
AT sisterorobertofelix thermaldecouplinginwumabinarysystems
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