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A 3D kinematic model of NGC 3242
Published online by Cambridge University Press: 25 May 2016
Extract
TAURUS-II imaging Fabry-Perot data in the emission lines of Ha, He II, [O I], [O III] and [N II] have been obtained to study the kinematics of NGC 3242. By studying the kinematic structure in lines of a range of ionization, the expansion of the nebula from close to the central star to the low ionization outer regions can be explored.
- Type
- IV. Envelopes
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- Copyright © Kluwer 1997
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