Broad-band polarization in crowded spectra

Details Broad-band polarization in crowded spectra Broad-band polarization in crowded spectra

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...237..237l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 237, no. 1, Oct. 1990, p. 237-242.

Astronomy and Astrophysics

Astrophysics

12

Interstellar Magnetic Fields, Polarization, Solar Spectra, Zeeman Effect, Absorption Spectra, Broadband, Late Stars, Spectral Line Width, Starspots, Sun

Scientific paper

The polarization due to differential saturation of Zeeman components is noticeably reduced in blended lines. Therefore, the polarization cannot increase very much in a crowded spectrum even though the fraction of the continuum subtracted by lines is larger and larger. Here, the influence of blends on K-type spectra is discussed. Arcturus is considered as an example.

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