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....
Guardado en:
| Autores principales: | , |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/141512 |
| Aporte de: |
| id |
I19-R120-10915-141512 |
|---|---|
| record_format |
dspace |
| 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 |
| _version_ |
1807220679520550912 |