Staff View: Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

Bibliographic Details
Main Authors:	Ribas, I., Jordi, C., Gimenez, A., Claret, A., Guinan, E. F.
Format:	Villanova Faculty Authorship
Language:	English
Published:	1999
Online Access:	http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176565

Main Authors:

Ribas, I., Jordi, C., Gimenez, A., Claret, A., Guinan, E. F.

Format:

Villanova Faculty Authorship

Language:

English

Published:

1999

Online Access:

http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176565

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spelling	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries. Ribas, I. Jordi, C. Gimenez, A. Claret, A. Guinan, E. F. Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication we focus on the comparison of observational data and model predictions for a sample of evolved eclipsing binaries, i.e. with components close to or beyond the TAMS, with the aim of studying the significance of convective core overshoot. 1999 Villanova Faculty Authorship vudl:176565 ASP Conference Series 173, 1999. en
dc.title_txt_mv	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
dc.creator_txt_mv	Ribas, I. Jordi, C. Gimenez, A. Claret, A. Guinan, E. F.
dc.description_txt_mv	Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication we focus on the comparison of observational data and model predictions for a sample of evolved eclipsing binaries, i.e. with components close to or beyond the TAMS, with the aim of studying the significance of convective core overshoot.
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author	Ribas, I. Jordi, C. Gimenez, A. Claret, A. Guinan, E. F.
spellingShingle	Ribas, I. Jordi, C. Gimenez, A. Claret, A. Guinan, E. F. Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
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description	Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication we focus on the comparison of observational data and model predictions for a sample of evolved eclipsing binaries, i.e. with components close to or beyond the TAMS, with the aim of studying the significance of convective core overshoot.
title	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
title_full	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
title_fullStr	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
title_full_unstemmed	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
title_short	Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
title_sort	test of convective core overshooting using evolved eclipsing binaries.
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Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.
Ribas, I.
Jordi, C.
Gimenez, A.
Claret, A.
Guinan, E. F.
Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication we focus on the comparison of observational data and model predictions for a sample of evolved eclipsing binaries, i.e. with components close to or beyond the TAMS, with the aim of studying the significance of convective core overshoot.
1999
Villanova Faculty Authorship
vudl:176565
ASP Conference Series 173, 1999.
en

dc.title_txt_mv

Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

dc.creator_txt_mv

Ribas, I.
Jordi, C.
Gimenez, A.
Claret, A.
Guinan, E. F.

dc.description_txt_mv

Double-lined eclipsing binaries are known to be the source of accurate stellar dimensions. Masses of radii of the component stars can be obtained with uncertainties around 1-2%, thus leading to the much-needed test of current models for stellar structure and evolution. In the present communication we focus on the comparison of observational data and model predictions for a sample of evolved eclipsing binaries, i.e. with components close to or beyond the TAMS, with the aim of studying the significance of convective core overshoot.

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author

Ribas, I.
Jordi, C.
Gimenez, A.
Claret, A.
Guinan, E. F.

spellingShingle

Ribas, I.
Jordi, C.
Gimenez, A.
Claret, A.
Guinan, E. F.
Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

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Jordi, C.
Gimenez, A.
Claret, A.
Guinan, E. F.

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Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

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Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

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Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

title_full_unstemmed

Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

title_short

Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

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test of convective core overshooting using evolved eclipsing binaries.

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Test of Convective Core Overshooting Using Evolved Eclipsing Binaries.

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