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- W1991932912 abstract "If the ion C IV is radiatively excited in a planetary nebula, three of its emission lines should be polarized when observed with a slit spectrograph in a suitable position with respect to the nebular image. One of the lines, λ3936, should be observable and perhaps should also be strong enough to allow the detection of its polarization." @default.
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- W1991932912 date "1972-04-01" @default.
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- W1991932912 title "Polarization of C IV Emission Lines in Planetary Nebulae" @default.
- W1991932912 doi "https://doi.org/10.1093/mnras/157.1.115" @default.
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