Line identifications in a fireball spectrum

Details Line identifications in a fireball spectrum Line identifications in a fireball spectrum

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..103...83b&link_type=abstract

Astronomy and Astrophysics Suppl. 103, 83-96 (1994)

Astronomy and Astrophysics

Astrophysics

16

Scientific paper

305 emission lines were found in a spectrum of a fireball of -9th magnitude. The identification of most of the lines is given. Also a detailed tracing of the spectrum in the range 3600 - 6600 A is presented. The tracing contains also computed synthetic spectrum and both spectra can be easily compared. The following species were found in the spectrum: Fe I, Na I, Mg I, Al I, Ca I, Ti I, Cr I, Mn I, Ni I, Mg II, Si II, Ca II, Fe II, FeO, probably also Si I, Ba II, C_2_, and possibly V I, Co I, Cu I, Ti II. The presence of other chemical elements in meteor spectra is discussed.

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