Chemical composition of the filaments in the Crab Nebula. I - Observed features in the spectra of the filaments

Astronomy and Astrophysics – Astrophysics

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Astronomical Spectroscopy, Chemical Composition, Crab Nebula, Spectrum Analysis, Forbidden Transitions, H Beta Line, Supernova Remnants

Scientific paper

An analysis of the available published spectroscopic observations of the Crab nebula filaments has been carried out. It has been shown that the relative intensities of the emission lines differ rather strongly from filament to filament, and these differences are real. The regularity in the observed variety of spectra has been studied. Owing to the regularity, the range of intensities of the observed lines is represented by means of three average spectra containing the intensities of all necessary lines.

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