CN, C2, and C3 excitation rates to be employed for interpreting photometric observations of comets

Details CN, C2, and C3 excitation rates to be employed for interpreting photometric observations of comets CN, C2, and C3 excitation rates to be employed for interpreting photometric observations of comets

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...134l...4f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 134, no. 1, May 1984, p. L4-L6.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Photometry, Bandpass Filters, Carbon, Comets, Cyanogen, Fluorescence, Linear Filters, Normal Density Functions, Optical Filters, Radial Velocity

Scientific paper

Numerous sets of standard interference filters for comet photometry are now being used for measuring selected emissions of comets. Due to both the finite value of their bandpasses and the Swings effect, an "effective" excitation rate must be computed to convert observed brightnesses into column densities. This effect is studied in detail for the CN filters; some conclusions concerning the use of C2 and C3 filters are also deduced.

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