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Infrared Astronomy

  • Chapter
Allen’s Astrophysical Quantities

Abstract

The Planck function in wavelength units (λμm in μm; T in K) is

$${B_{\lambda }} = 2h{c^{2}}{\lambda ^{{ - 5}}}/\left( {{e^{{hc/k\lambda T}}} - 1} \right)$$
$$= 1.1910 \times {10^{8}}\lambda _{{\mu m}}^{{ - 5}}/({e^{{14387.7/\lambda \mu mT}}} - 1)W{m^{{ - 2}}}\mu {m^{{ - 1}}}s{r^{{ - 1}}}$$

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    Arthur N. Cox

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Tokunaga, A.T. (2002). Infrared Astronomy. In: Cox, A.N. (eds) Allen’s Astrophysical Quantities. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-1186-0_7

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