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Christer Watson edited Analysis.tex  over 9 years ago

Commit id: 15e530f037c1277c90f6034481b31a23e48484f1

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where $\beta$ is assumed to be 2. The total column density is then:  \begin{equation}  N = \frac{I}{B_\nu \mu_H m_H \kappa R_d}\\  B_\nu = \frac{2 h \nu^3}{c^2 (e^\frac{h\nu}{kT}-1)\\ (e^\frac{h \nu}{kT}-1)}\\  %I = flux(at 350 \mu m)1.085\times 10^{-18} \left(\frac{18.6"}{\theta}\right)^2  \end{equation}