Abstract
Photometry in [OIII] emission of Planetary Nebulae in external galaxies can be used to determine distances as great as that of the Virgo cluster and beyond, as forcefully argued elsewhere during this conference (G.H. Jacoby, invited talk). In addition, measurement of the radial velocities of the PN allows dynamical behaviour to be probed to much greater distance from the galaxian centre than integrated light techniques (e.g. Arnaboldi 1994).
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References
M. Arnaboldi, K.C. Freeman, X. Hui, M. Capaccioli & H. Ford ESO Messenger, No. 76, pp. 40-44 (1994)
Taylor, K. and Douglas, N.G., IAU 149 ASP Conference Series, Vol. 71, pp. 33-37 (1995)
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© 1997 Springer Science+Business Media Dordrecht
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Douglas, N.G., Taylor, K., Freeman, K.C., Axelrod, T.S. (1997). A Dedicated Camera For Extragalactic Planetary Nebulae: The Planetary Nebula Spectrograph. In: Habing, H.J., Lamers, H.J.G.L.M. (eds) Planetary Nebulae. International Astronimical Union / Union Astronomique Internationale, vol 180. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5244-0_219
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DOI: https://doi.org/10.1007/978-94-011-5244-0_219
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