Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-02T18:41:11.214Z Has data issue: false hasContentIssue false
  • English
  • Français

IR Fabry-Perot imaging of NGC 3132

Published online by Cambridge University Press:  25 May 2016

L. E. Allen ,
M.C.B. Ashley ,
S. D. Ryder ,
J.W.V. Storey ,
Y-S. Sun  and
M. G. Burton
L. E. Allen
Affiliation:
University of New South Wales
M.C.B. Ashley
Affiliation:
University of New South Wales
S. D. Ryder
Affiliation:
University of New South Wales
J.W.V. Storey
Affiliation:
University of New South Wales
Y-S. Sun
Affiliation:
University of New South Wales
M. G. Burton
Affiliation:
University of New South Wales

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.

Near-infrared (1-3μm) emission lines of molecular and ionized hydrogen are excellent tools for investigating the morphology, energetics and kinematics of planetary nebulae, especially those PNe which contain large amounts of dust and are thus obscured at shorter wavelengths. The southern planetary nebula NGC 3132 was imaged with UNSWIRF (University of New South Wales Infrared Fabry-Perot) and IRIS on the 3.9m AAT Images in the H2 v=1-0 S(1) and H2 v=2-1 S(1) lines at 2.12μm and 2.25μm, and in Hii Brγ at 2.16μm are presented.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 205
Copyright
Copyright © Kluwer 1997