build based on a2ecdd1

dev/.documenter-siteinfo.json

@@ -1 +1 @@
-{"documenter":{"julia_version":"1.9.4","generation_timestamp":"2024-01-03T13:56:11","documenter_version":"1.2.1"}}
+{"documenter":{"julia_version":"1.9.4","generation_timestamp":"2024-01-05T15:15:01","documenter_version":"1.2.1"}}

dev/11_instructions/index.html

@@ -34,4 +34,4 @@
   [...]
     Grid1_file_dir = 'grid_png_20Msun_Z2d-2'
   [...]
-/</code></pre></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../9_homology_problems/">« Exercises</a><a class="docs-footer-nextpage" href="../11_questions/">Questions »</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option><option value="auto">Automatic (OS)</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.2.1 on <span class="colophon-date" title="Wednesday 3 January 2024 13:56">Wednesday 3 January 2024</span>. Using Julia version 1.9.4.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>
+/</code></pre></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../9_homology_problems/">« Exercises</a><a class="docs-footer-nextpage" href="../11_questions/">Questions »</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option><option value="auto">Automatic (OS)</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.2.1 on <span class="colophon-date" title="Friday 5 January 2024 15:14">Friday 5 January 2024</span>. Using Julia version 1.9.4.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>

dev/11_questions/index.html

@@ -84,4 +84,4 @@
    Dutch_wind_lowT_scheme = 'de Jager'
    Dutch_scaling_factor = 1.0  
    [...]
-/</code></pre><p>The <code>Dutch</code> prescription from MESA combines multiple prescriptions for mass loss from mostly Dutch authors, including those of <sup class="footnote-reference"><a id="citeref-deJager1988" href="#footnote-deJager1988">[deJager1988]</a></sup>, <sup class="footnote-reference"><a id="citeref-NugisLamers2000" href="#footnote-NugisLamers2000">[NugisLamers2000]</a></sup> and <sup class="footnote-reference"><a id="citeref-Vink2001" href="#footnote-Vink2001">[Vink2001]</a></sup>. A very important thing to keep in mind regarding mass loss rates in stellar evolution calculations is that they are based off prescriptions provided by other authors who have either determined them empirically or through dynamical modelling of stellar atmospheres, which is beyond the capabilities of MESA.</p><p>With your simulation completed, answer the following questions for your report:</p><ul><li>How does the onset of helium burning differ from the 2 Msun star modelled in the previous part?</li><li>Determine the time between the end of each burning phase (H, He, C, Ne, O, Si, core collapse). Compare it to the main-sequence lifetime.</li><li>At the end of your simulation, check the iron core-mass (fe<em>core</em>mass in your history file). Is there a relevance to that value?</li><li>From the profile at the end of your simulation plot the helium abundance across the entire star. Can you explain what is happening at the core?</li></ul><p>⏰ Time for the simulations: ~ 25mins in total ⏰</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Reimers1975"><a class="tag is-link" href="#citeref-Reimers1975">Reimers1975</a>Memoires of the Societe Royale des Sciences de Liege, Volume 8, pp. 369-382 (1975). https://ui.adsabs.harvard.edu/abs/1975MSRSL...8..369R/abstract</li><li class="footnote" id="footnote-Bloecker1995"><a class="tag is-link" href="#citeref-Bloecker1995">Bloecker1995</a>Astronomy and Astrophysics, Volume 297, pp. 727 (1995). https://ui.adsabs.harvard.edu/abs/1995A%26A...297..727B/abstract</li><li class="footnote" id="footnote-deJager1988"><a class="tag is-link" href="#citeref-deJager1988">deJager1988</a>Astronomy and Astrophysics, Suppl. Ser., Vol. 72, p. 259-289 (1988). https://ui.adsabs.harvard.edu/abs/1988A%26AS...72..259D/abstract</li><li class="footnote" id="footnote-NugisLamers2000"><a class="tag is-link" href="#citeref-NugisLamers2000">NugisLamers2000</a>Astronomy and Astrophysics, Vol. 360, p.227-244 (2000). https://ui.adsabs.harvard.edu/abs/2000A&amp;A...360..227N</li><li class="footnote" id="footnote-Vink2001"><a class="tag is-link" href="#citeref-Vink2001">Vink2001</a>Astronomy and Astrophysics, v.369, p.574-588 (2001). https://ui.adsabs.harvard.edu/abs/2001A%26A...369..574V/abstract</li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../11_instructions/">« Instructions</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option><option value="auto">Automatic (OS)</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.2.1 on <span class="colophon-date" title="Wednesday 3 January 2024 13:56">Wednesday 3 January 2024</span>. Using Julia version 1.9.4.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>
+/</code></pre><p>The <code>Dutch</code> prescription from MESA combines multiple prescriptions for mass loss from mostly Dutch authors, including those of <sup class="footnote-reference"><a id="citeref-deJager1988" href="#footnote-deJager1988">[deJager1988]</a></sup>, <sup class="footnote-reference"><a id="citeref-NugisLamers2000" href="#footnote-NugisLamers2000">[NugisLamers2000]</a></sup> and <sup class="footnote-reference"><a id="citeref-Vink2001" href="#footnote-Vink2001">[Vink2001]</a></sup>. A very important thing to keep in mind regarding mass loss rates in stellar evolution calculations is that they are based off prescriptions provided by other authors who have either determined them empirically or through dynamical modelling of stellar atmospheres, which is beyond the capabilities of MESA.</p><p>With your simulation completed, answer the following questions for your report:</p><ul><li>How does the onset of helium burning differ from the 2 Msun star modelled in the previous part?</li><li>Determine the time between the end of each burning phase (H, He, C, Ne, O, Si, core collapse). Compare it to the main-sequence lifetime.</li><li>At the end of your simulation, check the iron core-mass (fe<em>core</em>mass in your history file). Is there a relevance to that value?</li><li>From the profile at the end of your simulation plot the helium abundance across the entire star. Can you explain what is happening at the core?</li></ul><p>⏰ Time for the simulations: ~ 25mins in total ⏰</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Reimers1975"><a class="tag is-link" href="#citeref-Reimers1975">Reimers1975</a>Memoires of the Societe Royale des Sciences de Liege, Volume 8, pp. 369-382 (1975). https://ui.adsabs.harvard.edu/abs/1975MSRSL...8..369R/abstract</li><li class="footnote" id="footnote-Bloecker1995"><a class="tag is-link" href="#citeref-Bloecker1995">Bloecker1995</a>Astronomy and Astrophysics, Volume 297, pp. 727 (1995). https://ui.adsabs.harvard.edu/abs/1995A%26A...297..727B/abstract</li><li class="footnote" id="footnote-deJager1988"><a class="tag is-link" href="#citeref-deJager1988">deJager1988</a>Astronomy and Astrophysics, Suppl. Ser., Vol. 72, p. 259-289 (1988). https://ui.adsabs.harvard.edu/abs/1988A%26AS...72..259D/abstract</li><li class="footnote" id="footnote-NugisLamers2000"><a class="tag is-link" href="#citeref-NugisLamers2000">NugisLamers2000</a>Astronomy and Astrophysics, Vol. 360, p.227-244 (2000). https://ui.adsabs.harvard.edu/abs/2000A&amp;A...360..227N</li><li class="footnote" id="footnote-Vink2001"><a class="tag is-link" href="#citeref-Vink2001">Vink2001</a>Astronomy and Astrophysics, v.369, p.574-588 (2001). https://ui.adsabs.harvard.edu/abs/2001A%26A...369..574V/abstract</li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../11_instructions/">« Instructions</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option><option value="auto">Automatic (OS)</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.2.1 on <span class="colophon-date" title="Friday 5 January 2024 15:14">Friday 5 January 2024</span>. Using Julia version 1.9.4.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>