Hostname: page-component-76fb5796d-x4r87 Total loading time: 0 Render date: 2024-04-26T01:41:58.326Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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