Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1969
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...5..323v&link_type=abstract
Astrophysics and Space Science, Volume 5, Issue 3, pp.323-332
Astronomy and Astrophysics
Astrophysics
25
Scientific paper
The excitation temperature, colour excess and continuum of η Car in the visible and near ultraviolet have been determined from the study of the excitation of the ionized iron emission lines. The excitation temperatures of Fe ii and [Fe ii] are about 8000K, value which is very much lower than the mean ionization temperature of the elements in η Car.E B-V is about 1m.1; the absolute visual magnitude is presently -10m.5±1m. From the equivalent widths of the emission lines the true continuum between 1.5 and 3.0 μ-1 has been derived. The correspondingB-V is -0m.14, while the Balmer jump is less than 0m.5. The continuum appears mainly nebular in origin with a strong contribution of the two-photon emission from the 2s-level of hydrogen in the blue.
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