Monochromatic observations of planetary nebulae |
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Authors: | R. Louise C. T. Hua |
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Affiliation: | (1) Laboratoire de Physique Théorique, Faculté des Sciences, Amiens, France;(2) Laboratoire d'Astronomie Spatiale, Traverse du Siphon, Marseille, France |
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Abstract: | ![]() Monochromatic images in H , H , [Nii] 6584, [Sii] 6717, and [Oiii] 5007 lines are presented for a morphological study of planetary nebulae. Narrow bandpass ( =5 to 10Å) interference filters are generally used in order to discriminate peculiar structures existing in different emission lines. However, large bandwidths ( =50 Å) along with long exposures, are also necessary in searching for faint nebulosities associated with planetaries.Three faint objects of the Abell's list of old planetary nebulae have been observed through narrow band filters, by means of an image tube (A33, A36 in Chile) or the image photon counting device (A79 at the Haute Provence Observatory). Following the H /[Nii] intensity ratio, a discussion is given about the distance previously derived with some assumptions concerning the measured red fluxes. |
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