Abstract
The planetary nebula Hubble 5 shows a very striking bi-symmetry; a 180° rotation around its center would bring the object into fair coincidence. Similar to this nebula is NGC 6537 and, to a lesser degree, NGC 6302. Jet outflows are reported from this “post-main sequence” nebula over a range of 260 km s-1 (Phillips and Mampaso, 1988). Otherwise not much has appeared on this object in the literature.
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© 1993 Springer Science+Business Media Dordrecht
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Pişmiş, P., Manteiga, M., Mampaso, A., Cruz-Gonzalez, G. (1993). Kinematics of the Planetary Nebula Hb 5.. In: Weinberger, R., Acker, A. (eds) Planetary Nebulae. International Astronomical Union / Union Astronomique Internationale, vol 155. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2088-3_74
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DOI: https://doi.org/10.1007/978-94-011-2088-3_74
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