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1999ApJ...525..863F - Astrophys. J., 525, 863-870 (1999/November-2)
The IUE spectra of the O VI sequence planetary nebulae NGC 2452, NGC 7026, M3-30, and Lo 4.
FEIBELMAN W.A.
Abstract (from CDS):
We present emission-line fluxes for NGC 2452, NGC 7026, M3-30, and Lo 4 from IUE low-dispersion spectra that have been processed by the New Spectral Image Processing System (NEWSIPS). For NGC 2452, a terminal wind velocity of -4200±300 km.s–1 was determined from the C IV λ1549 P Cygni profile, while that of NGC 7026 is -4600±300 km.s–1, and -4800±400 km.s–1 for M3-30. The spectrum of Lo 4 is a stellar continuum with some absorptions and a questionable C IV λ1549 feature.
Abstract Copyright: ∼
Journal keyword(s): planetary nebulae: individual (NGC 2452, NGC 7026, M3-30, Lo 4) - Ultraviolet: ISM
Simbad objects: 27
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