Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-03T01:38:20.229Z Has data issue: false hasContentIssue false

Millimeter-Wave Observations of Planetary Nebulae

Published online by Cambridge University Press:  22 September 2016

Hugh M. Johnson*
Affiliation:
Lockheed Missiles and Space Co. Palo Alto, California

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.

Observations of the integrated continuum flux density of several stellar planetary nebulae have been made at 90 GHz. These are reported, with some remarks on their significance for objects with positive radio-frequency spectral index, and to display graphically their relation to published microwave and near-infrared data. The 90-GHz data have been obtained with the 11-m dish of the National Radio Astronomy Observatory* on Kitt Peak, under the Lockheed Independent Research Program. Three of the objects have been included among a dozen stellar planetary nebulae observed with the Fabry-Perrot interferometer at the Cerro Tololo Inter-American Observatoryt so as to provide kinematical information with the microwave spectral data, since they are related in the theories of the positive spectral index that appeared in 1975. The Fabry-Perot observations are reported in Astrophys. J. 1977 September 15. No other journal article is yet in press.

Type
Session VII: The Origin of Planetary Nebulaesession VII the Origin of Planetary Nebulae
Copyright
Copyright © Reidel 1978