H beta luminosities of planetary nebula central stars

Details H beta luminosities of planetary nebula central stars H beta luminosities of planetary nebula central stars

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222..147m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 147-155

Astronomy and Astrophysics

Astrophysics

3

Galactic Bulge, H Beta Line, Interstellar Extinction, Luminosity, Planetary Nebulae, Scaling Laws, Variable Stars, Mass Distribution, Optical Thickness, Stellar Magnitude, Stellar Temperature

Scientific paper

The determination of the luminosities of planetary nebula central stars from H beta nebular fluxes is investigated. A correlation is obtained with the luminosities derived from independent stellar parameters. An average scaling factor is determined for H beta luminosities of optically thick nebulae, as well as correlations of this parameter with the Zanstra He II and H I temperatures.

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