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Translation from the Portuguese language edition: Astrofίsica do Meio Interestelar by Walter J. Maciel © Editora da Universidade de São Paulo (Edusp). All rights reserved.
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PAGE 18, SECTION 2.2.1, SECOND PARAGRAPH
Plasma emissivity, defined as the total power emitted per unit volume per unit solid angle per unit frequency interval between ν e ν+ dν, is given by
and it is generally measured in erg cm−3 s−1 sr−1 Hz−1, where f(v) is the distribution function of electron velocities and P(v,ν) is the total power emitted per unit frequency interval during the collision between an electron with velocity v and an ion with density n i. If f(v) is given by the Maxwellian distribution, the emissivity is...
PAGE 57, AFTER EQUATION (4.13)
where we neglect the radiation intensity falling on the region opposite to the observer and τ νr is again the total optical depth of the emitting region...
PAGE 80, AFTER EQUATION (5.15)
From (5.6), we see that coefficient γ jk gives the collision probability per unit time per field particle so that nc γ jk gives the number of excitations per second, and the product nt nc γ jk gives the number of excitations per cubic centimeter per second, where nt is the test particle density...
PAGE 126, EQUATION (7.18)
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Maciel, W.J. (2013). Erratum. In: Astrophysics of the Interstellar Medium. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-3767-3_12
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DOI: https://doi.org/10.1007/978-1-4614-3767-3_12
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