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Pinpointing the position of the post-asymptotic giant branch star at the core of RAFGL 2688 using polarimetric imaging with NICMOSThe authors have used infrared polarimetric imaging with NICMOS to determine precisely the position of the star that illuminates (and presumably generated) the bipolar, preplanetary reflection nebula RAFGL 2688 (the Egg Nebula).
Document ID
20060033078
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/15653
Authors
Weintraub, D.
Kastner, J.
Hines, D.
Sahai, R.
Date Acquired
August 23, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Astrophysical Journal
Volume: 531
Issue: 1
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
Polarimetric imaging nicmos nebula

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