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A 3D kinematic model of NGC 3242

Published online by Cambridge University Press:  25 May 2016

G. Dudziak ,
J. R. Walsh  and
N. Walton
G. Dudziak
Affiliation:
1European Southern Observatory
J. R. Walsh
Affiliation:
1European Southern Observatory
N. Walton
Affiliation:
2Royal Greenwich Observatory, La Palma

Extract

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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
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 222
Copyright
Copyright © Kluwer 1997 

References

Barker, T., 1985, ApJ, 294, 193.CrossRefGoogle Scholar
Hajian, A.R., Terzian, Y., Bignell, C., 1995, AJ, 109, 2600.Google Scholar