this is for holding javascript data
Matteo Cantiello added We_quantify_the_mass_dependent__.tex
almost 9 years ago
Commit id: 2719196e4479f1eb1e787347338e0fb007559f25
deletions | additions
diff --git a/We_quantify_the_mass_dependent__.tex b/We_quantify_the_mass_dependent__.tex
new file mode 100644
index 0000000..3b8e107
--- /dev/null
+++ b/We_quantify_the_mass_dependent__.tex
...
We quantify the mass-dependent mode suppression in Fig. 3 by
showing the relative number of suppressed stars (those below the dashed
line in Fig. 2) in narrow mass intervals.
We see no suppressed stars below 1.1\msol, while above this threshold there
is first a gradual increase followed by a rapid increase above approximately
1.5\msol, and a drop beyond 2.0\msol.
The onset of suppression beyond 1.1\msol, coincides with the mass above
which stars are thought to form convective cores during their hydrogen-core
burning phase[REF].
We believe this shows evidence for the establishment of
convectively driven dynamos in the cores of low-mass hydrogen-core burning
stars [REF CharbonneauMacGregor01,MacgregorCassinelli03Brun05].
The gradual increase in suppression may result from the increasing size of
the convective core in more massive stars, which generates stronger
magnetic fields that survive after hydrogen burning ceases in the core.
[Jim/Matteo elaborate?]
