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IR Fabry-Perot imaging of NGC 3132

  • L. E. Allen (a1), M.C.B. Ashley (a1), S. D. Ryder (a1), J.W.V. Storey (a1), Y-S. Sun (a1) and M. G. Burton (a1)...

Extract

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.

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