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Spectroscopy and Three‐Dimensional Imaging of the Crab Nebula

  • Authors: Andrej Čadež, Alberto Carramiñana, and Simon Vidrih

Čadež, CarramiÑana, & Vidrih 2004 The Astrophysical Journal 609 797.

  • Provider: AAS Journals

Caption: Fig. 10.

Same as Fig. 9 for the high‐resolution spectra. The S/N for this spectroscopy is quite low (see text), so that some specks are due to noise fluctuations; in particular, the trace ﹩\psi =18^{\circ }﹩ is the noisiest, since it has the lowest maximum intensity (see text). This spectroscopy is mainly useful in conjunction with low‐resolution spectroscopy for better velocity calibration. Compare also with Fig. 2.

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