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The Complex Environment of the High Excitation Planetary Nebula NGC 3242Spatially resolved profiles of the H (alpha), [N II] 6584 A and [O III] 5007 A nebular emission lines, obtained with the Manchester echelle spectrometer combined with the 2.1 m San Pedro Martir telescope have revealed the velocity structure of the nebular core and of one of the three (A,B and C) inner haloes of the high excitation planetary nebula NGC 3242.
Document ID
20060040992
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/18672
Authors
Noriega-Crespo, A.
Meaburn, J.
Lopez, J.
Date Acquired
August 23, 2013
Publication Date
November 15, 1999
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
planetary nebulae NGC 3242 kinematics and dynamics haloes

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