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Kinematics of Abell 30
Published online by Cambridge University Press: 19 July 2016
Abstract
Abell 30 is a remarkable PN with a H-depleted core. Four bright knots have been identified in the [O III] line (Jacoby 1979). The previous kinematic study has shown that J1 and J3 form a pair expanding at radial velocities of ±25 km/s with respect to the central star, and J4 has a radial velocity of −22 km/s (Reay, Atherton, and Taylor 1983).
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- II. Nebular Properties
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- Copyright © Kluwer 1989
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