Numerically efficient expressions for nebular line cooling

Details Numerically efficient expressions for nebular line cooling Numerically efficient expressions for nebular line cooling

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...275..588b&link_type=abstract

Astronomy and Astrophysics, Vol. 275, p. 588 (1993)

Astronomy and Astrophysics

Astrophysics

7

Radiation Mechanisms: General, Interstellar Medium: General

Scientific paper

Optical and UV forbidden lines are some of the dominant radiative energy loss mechanisms in nebular astrophysics. Direct numerical calculations of their cooling rates are generally very time consuming. Computationally efficient polynomial approximations of important volume emissivities for various ions of C, N, O, Ne, and S are fitted and presented in the domain 1 ≤ log10(ne/cm-3) ≤ 7 and 3.5 ≤ log10(Te/K) ≤ 5.

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