Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-12T12:48:57.606Z Has data issue: false hasContentIssue false
  • English
  • Français

Millimetre and Submillimetre Continuum Observations of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

M.G. Hoare ,
P.F. Roche  and
R.E.S. Clegg
M.G. Hoare
Affiliation:
Astrophysics, Dept of Physics, Oxford University, Nuclear Physics Building, Keble Rd., Oxford 0X1 3RH, UK
P.F. Roche
Affiliation:
Astrophysics, Dept of Physics, Oxford University, Nuclear Physics Building, Keble Rd., Oxford 0X1 3RH, UK
R.E.S. Clegg
Affiliation:
Royal Greenwich Observatory, Madingley Rd, Cambridge CB3 0EZ, UK

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.

Continuum emission has been detected at millimetre and submillimetre wavelengths from a total of thirteen planetary nebulae, all but one for the first time. The observations were obtained with the liquid 3He–cooled UKT14 bolometer on the JCMT and UKIRT telescopes on Mauna Kea, Hawaii.

Type
III. Highlights on the Nebulae
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 232
Copyright
Copyright © Kluwer 1993