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that can be used to reproduce the panels of Figures 4-5.
The subdirectory 'matlab' contains MATLAB scripts (The Mathworks, USA) that can be used to reproduce the panels of Figures 4-5.
In the left hand panels of Figures 1 and 2, uanal x,0) and unum x,0) are drawn together in the same window.
In the left hand panels of Figures 3 and 4, both d dt u anal x, 0 Open image in new window and d dt u num x, 0 Open image in new windowu x,0) are shown together in the same window.
However, in contrast with the behaviour seen in the case of nonrotating stars, the dynamics of the low-density material in the stellar exterior results in a degradation of the conservation of mass for the EL5 scheme, as shown in the left panel of Figure 21 (cf., the left panels of Figures 12 and 14 for the equivalent behaviour in the absence of rotation).
As shown in the insets of left panels of Figures 3 and 4, the exponents n are 0 at 0 K and with an increase of temperature, n of SiNW approaches n=2 at around 100 K while that of DNW becomes n=2 at around 300 K.
Similar(21)
- 'Figure3.m': this script plots panels of figure 3.
- 'figure4.m': this script plots panels of figure 4.
- 'SuppFigure2.m': this script plots panels of figure S2.
- 'SuppFigure3.m': this script plots panels of figure S3.
- 'SuppFigure9.m': this script plots panels of figure S9.
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Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com