The ultraviolet spectrum of the planetary nebula NGC 6572

Details The ultraviolet spectrum of the planetary nebula NGC 6572 The ultraviolet spectrum of the planetary nebula NGC 6572

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.194p..13f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 194, Jan. 1981, p. 13P-16P.

Astronomy and Astrophysics

Astronomy

17

Carbon, H Lines, Iue, Planetary Nebulae, Ultraviolet Spectra, Abundance, Electron Recombination, Infrared Astronomy, Magnesium, Ultraviolet Astronomy, Visual Observation

Scientific paper

The ultraviolet emission line spectrum of NGC 6572 has been analyzed in
conjunction with visual and infrared observations of the nebula.
Particular attention is paid to the C/O abundance ratio for which a
value of 1.1 is derived. Gaseous Mg is found to be depleted in the outer
regions of the nebula.

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