The polarization of radiation in CH Cygni in quiet and active phases

Details The polarization of radiation in CH Cygni in quiet and active phases The polarization of radiation in CH Cygni in quiet and active phases

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...80r&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Jan.-Feb. 1989, p. 80-83, 89. In Russian.

Physics

Cool Stars, Giant Stars, Polarized Radiation, Stellar Activity, Symbiotic Stars, Dwarf Stars, Emission Spectra, Hot Stars, Stellar Spectrophotometry, Ultraviolet Radiation

Scientific paper

The polarization of the radiation in CH Cyg during 1974-1976 (a quiet phase) was characterized by a significant increase in the degree of polarization in UV spectral region; this is typical for many cool giants. In the active state (autumn of 1984), the degree of polarization decreased markedly in the UV. This may be due to the depolarizing effect of the emission lines.

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