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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code
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| Zeitschriftentitel: | Proceedings of the International Astronomical Union |
|---|---|
| Personen und Körperschaften: | , , , , |
| In: | Proceedings of the International Astronomical Union, 9, 2014, S307, S. 142-143 |
| Format: | E-Article |
| Sprache: | Englisch |
| veröffentlicht: |
Cambridge University Press (CUP)
|
| Schlagwörter: |
| author_facet |
Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. |
|---|---|
| author |
Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. |
| spellingShingle |
Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. Proceedings of the International Astronomical Union Revisiting the Hunter diagram with the Geneva Stellar Evolution Code Astronomy and Astrophysics Space and Planetary Science |
| author_sort |
simoniello, r. |
| spelling |
Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. 1743-9213 1743-9221 Cambridge University Press (CUP) Astronomy and Astrophysics Space and Planetary Science http://dx.doi.org/10.1017/s1743921314006589 <jats:title>Abstract</jats:title><jats:p>We produced a model grid of rotating main and post-main sequence stars with the Geneva Stellar Evolution Code (GENEC). The initial chemical composition is tailored to compare with observations of early OB type stars in the Large Magellanic Cloud (LMC) and the grid covers stellar masses in the range of 7 ≤ <jats:italic>M</jats:italic>/<jats:italic>M</jats:italic><jats:sub>⊙</jats:sub> ≤ 15 and initial velocity between 0 km s<jats:sup>−1</jats:sup> ≤ <jats:italic>v</jats:italic> sin(i) ≤ 300 km s<jats:sup>−1</jats:sup>. The model grid has been used to determine the changes in the surface Nitrogen abundances during the star evolution and the results have been compared with observations.</jats:p> Revisiting the Hunter diagram with the Geneva Stellar Evolution Code Proceedings of the International Astronomical Union |
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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
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Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_short |
Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_sort |
revisiting the hunter diagram with the geneva stellar evolution code |
| topic |
Astronomy and Astrophysics Space and Planetary Science |
| url |
http://dx.doi.org/10.1017/s1743921314006589 |
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2014 |
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142-143 |
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<jats:title>Abstract</jats:title><jats:p>We produced a model grid of rotating main and post-main sequence stars with the Geneva Stellar Evolution Code (GENEC). The initial chemical composition is tailored to compare with observations of early OB type stars in the Large Magellanic Cloud (LMC) and the grid covers stellar masses in the range of 7 ≤ <jats:italic>M</jats:italic>/<jats:italic>M</jats:italic><jats:sub>⊙</jats:sub> ≤ 15 and initial velocity between 0 km s<jats:sup>−1</jats:sup> ≤ <jats:italic>v</jats:italic> sin(i) ≤ 300 km s<jats:sup>−1</jats:sup>. The model grid has been used to determine the changes in the surface Nitrogen abundances during the star evolution and the results have been compared with observations.</jats:p> |
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| author | Simoniello, R., Meynet, G., Ekström, S., Georgy, C., Granada, A. |
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| description | <jats:title>Abstract</jats:title><jats:p>We produced a model grid of rotating main and post-main sequence stars with the Geneva Stellar Evolution Code (GENEC). The initial chemical composition is tailored to compare with observations of early OB type stars in the Large Magellanic Cloud (LMC) and the grid covers stellar masses in the range of 7 ≤ <jats:italic>M</jats:italic>/<jats:italic>M</jats:italic><jats:sub>⊙</jats:sub> ≤ 15 and initial velocity between 0 km s<jats:sup>−1</jats:sup> ≤ <jats:italic>v</jats:italic> sin(i) ≤ 300 km s<jats:sup>−1</jats:sup>. The model grid has been used to determine the changes in the surface Nitrogen abundances during the star evolution and the results have been compared with observations.</jats:p> |
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| imprint_str_mv | Cambridge University Press (CUP), 2014 |
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| physical | 142-143 |
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| series | Proceedings of the International Astronomical Union |
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| spelling | Simoniello, R. Meynet, G. Ekström, S. Georgy, C. Granada, A. 1743-9213 1743-9221 Cambridge University Press (CUP) Astronomy and Astrophysics Space and Planetary Science http://dx.doi.org/10.1017/s1743921314006589 <jats:title>Abstract</jats:title><jats:p>We produced a model grid of rotating main and post-main sequence stars with the Geneva Stellar Evolution Code (GENEC). The initial chemical composition is tailored to compare with observations of early OB type stars in the Large Magellanic Cloud (LMC) and the grid covers stellar masses in the range of 7 ≤ <jats:italic>M</jats:italic>/<jats:italic>M</jats:italic><jats:sub>⊙</jats:sub> ≤ 15 and initial velocity between 0 km s<jats:sup>−1</jats:sup> ≤ <jats:italic>v</jats:italic> sin(i) ≤ 300 km s<jats:sup>−1</jats:sup>. The model grid has been used to determine the changes in the surface Nitrogen abundances during the star evolution and the results have been compared with observations.</jats:p> Revisiting the Hunter diagram with the Geneva Stellar Evolution Code Proceedings of the International Astronomical Union |
| spellingShingle | Simoniello, R., Meynet, G., Ekström, S., Georgy, C., Granada, A., Proceedings of the International Astronomical Union, Revisiting the Hunter diagram with the Geneva Stellar Evolution Code, Astronomy and Astrophysics, Space and Planetary Science |
| title | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_full | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_fullStr | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_full_unstemmed | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_short | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| title_sort | revisiting the hunter diagram with the geneva stellar evolution code |
| title_unstemmed | Revisiting the Hunter diagram with the Geneva Stellar Evolution Code |
| topic | Astronomy and Astrophysics, Space and Planetary Science |
| url | http://dx.doi.org/10.1017/s1743921314006589 |