Tools of Radio Astronomy pp 151-157 | Cite as
Solutions for Chapter 14
Chapter
Abstract
For an ideal gas, we have PV = NkT. With N/V = n, the pressure becomes P = nkT. For standard laboratory conditions, the density is: n = 2.65 × 1019cm−3.
Keywords
Line Intensity Molecular Cloud Radiative Decay Column Density Boltzmann Distribution
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© Springer-Verlag Berlin Heidelberg 2000