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A Comparison of Radio-Frequency and Optical Studies of Selected Planetary Nebulae
Published online by Cambridge University Press: 25 April 2016
Extract
The thermal radio-frequency emission, Ev, per unit volume per unit frequency interval may be computed (e.g. from equations given by Oster) and compared with the volume emissivity E(Hβ) in the optical Hβ transition.
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- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 1 , Issue 6 , September 1969 , pp. 283 - 285
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- Copyright © Astronomical Society of Australia 1969