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The UV emission line spectrum of NGC 6572Ultraviolet spectra of the medium excitation planetary nebula NGC 6572 were obtained with IUE both in the low and in the high resolution mode. These spectra reveal a superposition of emission lines arising in the expanding atmosphere of the central star, evidenced e.g., by their P Cygni profiles, and features arising in the planetary nebula proper. The latter were analyzed in order to determine C, N, O abundances.
Document ID
19820023349
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Grewing, M. (Tuebingen Univ.)
Kraemer, G. (Tuebingen Univ.)
Preussner, P. R. (Tuebingen Univ.)
Schulz-Luepertz, E. (Tuebingen Univ.)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31225
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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