The O VI nucleus of the planetary nebula M3-30

Details The O VI nucleus of the planetary nebula M3-30 The O VI nucleus of the planetary nebula M3-30

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...278..195k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 278, March 1, 1984, p. 195-200.

Other

29

Oxygen Spectra, Planetary Nebulae, Stellar Luminosity, Stellar Spectra, Carbon, Helium, Line Spectra, Stellar Temperature

Scientific paper

The discovery of another star with powerful O IV emission, the nucleus of the planetary nebula M3-30, is reported, along with quantitative measurements of the strength of the line relative to the luminosity of the star. This information is essential to determine how the O IV nuclei fit into the general scheme of planetary evolution. For comparison, estimates of the same quantities are made for other O IV stars from data found in the literature. Except for the generally high luminosities and temperatures of the stars, no correlation can be found between O IV strength and position on the log L-log T plane, which may reflect the generally poor state of the available data.

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