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The changing spectrum of the LMC planetary N66Recent spectroscopy and photometry of the planetary nebula N66 (SMP 83) in the Large Magellanic Cloud show a continuing evolution, with a central WR spectrum becoming more visible. The planetary nebula shell and Wolf-Rayet (WR) star have velocities which differ by approximately 240 km/s. Properties of this interesting object are reviewed, and we discuss its possible X-ray detection by ROSAT.
Document ID
19950054644
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/133455
Authors
Cowley, A. P. (Arizona State University Tempe, AZ, United States)
Crampton, D. (Herzberg Institute of Astrophysics Victoria, BC, Canada)
Schmidtke, P. C. (Arizona State University Tempe, AZ, United States)
Mcgrath, T. K. (Arizona State University Tempe, AZ, United States)
Hutchings, J. B. (Herzberg Institute of Astrophysics Victoria, BC, Canada)
Date Acquired
August 16, 2013
Publication Date
August 1, 1994
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 106
Issue: 702
ISSN: 0004-6280
Subject Category
Astronomy
Accession Number
95A86243
Distribution Limits
Public
Copyright
Other

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