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lines changed Original file line number Diff line number Diff line change 693693 "metadata" : {},
694694 "source" : [
695695 " Spectroscopically, MN Lup is classified as spectral type M0 V, thus\n " ,
696- " the gravitational acceleration on the surface :math:` \\ log(g)` \n " ,
696+ " the gravitational acceleration on the surface $ \\ log(g)$ \n " ,
697697 " should be comparable to the sun.\n " ,
698698 " (For non-stellar astronomers: Conventionally, all values are given\n " ,
699- " in the cgs system. The value for the sun is :math:` \\ log(g) = 4.4` .)\n " ,
699+ " in the cgs system. The value for the sun is $ \\ log(g) = 4.4$ .)\n " ,
700700 " \n " ,
701- " Calculate :math:` \\ log(g)` for MN Lup with the values for the mass\n " ,
701+ " Calculate $ \\ log(g)$ for MN Lup with the values for the mass\n " ,
702702 " and radius given above. Those values were determined from\n " ,
703- " evolutionary tracks. Check if the :math:` \\ log(g)` is consistent\n " ,
703+ " evolutionary tracks. Check if the $ \\ log(g)$ is consistent\n " ,
704704 " with the value expected from spectroscopy"
705705 ]
706706 },
758758 "metadata" : {},
759759 "source" : [
760760 " You can test if you function works by calculating the a Dopplershift\n " ,
761- " of the following wavelengths relative to :math:` H_\\ alpha` "
761+ " of the following wavelengths relative to $ H_\\ alpha$ "
762762 ]
763763 },
764764 {
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