Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-25T19:39:24.213Z Has data issue: false hasContentIssue false

Measurements on Planetary Nebulae

Published online by Cambridge University Press:  14 August 2015

D. K. Milne
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia
L. H. Aller
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

Abstract

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.

165 planetary nebulae south of +27° declination have been observed with the Parkes 64 m telescope. These nebulae were chosen to include most of those for which Hβ flux densities are available. Radio positions and flux densities (generally with probable errors of only a few millijanskies) obtained from the survey must represent the most reliable and homogeneous radio data currently available for the class of object. The data have been used to obtain distances and optical extinctions for these nebulae.

Type
Part 4: Stellar and Circumstellar Sources
Copyright
Copyright © Reidel 1974 

References

Aller, L. H. and Milne, D. K.: 1972, Australian J. Phys. 25, 91.CrossRefGoogle Scholar
Gurzadyan, G. A.: 1963, Soobshch. Byurakansk. Obs. Akad. Nauk Arm. S.S.R. 34, 59.Google Scholar
Metik, L. P. and Gershberg, R. E.: 1964, Izv. Krymsk. Astrofiz. Obs. 31, 112.Google Scholar
Minkowski, R. and Aller, L. H.: 1954, Astrophys. J. 120, 261.Google Scholar
Mottmann, J.: 1972, Thesis, University of California, Los Angeles.Google Scholar
Shklovskii, I. S.: 1956, Astron. Zh. 33, 222.Google Scholar