The IUE Spectra of the O VI Sequence Planetary Nebulae NGC 2452, NGC 7026, M3-30, and Lo 4

Details The IUE Spectra of the O VI Sequence Planetary Nebulae NGC 2452, NGC 7026, M3-30, and Lo 4 The IUE Spectra of the O VI Sequence Planetary Nebulae NGC 2452, NGC 7026, M3-30, and Lo 4

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999apj...525..863f&link_type=abstract

The Astrophysical Journal, Volume 525, Issue 2, pp. 863-870.

Astronomy and Astrophysics

Astronomy

2

Planetary Nebulae: Individual (Ngc 2452, Ngc 7026, M3-30, Lo 4), Ultraviolet: Ism

Scientific paper

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.

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