wip

Author: gnthibault

Physics101StarSpectroscopyLines.ipynb

@@ -29,6 +29,22 @@
     "#IFrame(\"doc/Physics/star_spectro_intro.pdf\", width=1200, height=800)"
    ]
   },
+  {
+   "cell_type": "code",
+   "execution_count": null,
+   "metadata": {},
+   "outputs": [],
+   "source": []
+  },
+  {
+   "cell_type": "markdown",
+   "metadata": {},
+   "source": [
+    "## Why spectroscopy lines should be modeled as Lorentzian functions\n",
+    "\n",
+    "This introduction directly inspired by the [wikipedia article](https://en.wikipedia.org/wiki/Cauchy_distribution)"
+   ]
+  },
   {
    "cell_type": "code",
    "execution_count": null,