No CrossRef data available.
Article contents
The electron density in the plane of the Galaxy
Published online by Cambridge University Press: 04 August 2017
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Pulsars provide probably the best probes of electron density in the plane of the Galaxy. The dispersion measure, the path integral of electron density along the line of sight from the pulsar to Earth, ∫ neds, is directly measurable from multi-frequency pulse-timing observations. The distance to a pulsar, d, can be estimated from its HI absorption and emission spectra. The mean electron density along the line of sight is then just <ne> = ∫ neds/d.
- Type
- PART II: COMPOSITION, STRUCTURE AND KINEMATICS
- Information
- Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 181 - 182
- Copyright
- Copyright © Reidel 1985
References
Weisberg, J.M., Rankin, J., and Boriakoff, V.: 1980, Astron. Astrophys.
88, pp. 84–93
Google Scholar
You have
Access