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lines changed Original file line number Diff line number Diff line change 693
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"metadata" : {},
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"source" : [
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" Spectroscopically, MN Lup is classified as spectral type M0 V, thus\n " ,
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- " the gravitational acceleration on the surface :math:` \\ log(g)` \n " ,
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+ " the gravitational acceleration on the surface $ \\ log(g)$ \n " ,
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" should be comparable to the sun.\n " ,
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" (For non-stellar astronomers: Conventionally, all values are given\n " ,
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- " in the cgs system. The value for the sun is :math:` \\ log(g) = 4.4` .)\n " ,
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+ " in the cgs system. The value for the sun is $ \\ log(g) = 4.4$ .)\n " ,
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" \n " ,
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- " Calculate :math:` \\ log(g)` for MN Lup with the values for the mass\n " ,
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+ " Calculate $ \\ log(g)$ for MN Lup with the values for the mass\n " ,
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" and radius given above. Those values were determined from\n " ,
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- " evolutionary tracks. Check if the :math:` \\ log(g)` is consistent\n " ,
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+ " evolutionary tracks. Check if the $ \\ log(g)$ is consistent\n " ,
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" with the value expected from spectroscopy"
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]
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},
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"metadata" : {},
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"source" : [
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" You can test if you function works by calculating the a Dopplershift\n " ,
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- " of the following wavelengths relative to :math:` H_\\ alpha` "
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+ " of the following wavelengths relative to $ H_\\ alpha$ "
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]
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},
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{
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