Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-26T04:06:25.609Z Has data issue: false hasContentIssue false
  • English
  • Français

Long term trends in the 3.5 μ light curve of RX Puppis

Published online by Cambridge University Press:  12 April 2016

Patricia A. Whitelock  and
R.M. Catchpole
Patricia A. Whitelock
Affiliation:
South African Astronomical Observatory
R.M. Catchpole
Affiliation:
South African Astronomical Observatory

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.

SAAO photometry of RX Pup at 3.5 μ between 1972 and 1981 shows a very well defined period of 580 days with an amplitude of 0.35 mag, which is attributed to a Mira variable component. The infrared variability of RX Pup was demonstrated by Feast, Robertson and Catchpole (1977), who also pointed out that the infrared colours were indicative of the presence of a Mira variable with a dust excess. Further evidence for the Mira comes from the observations of H2O in the infrared spectrum by Barton, Phillips and Allen (1979).

Type
Session II – Discussion on Individual Stars
Information
International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 207 - 208
Copyright
Copyright © Reidel 1982

References

Barton, J.R., Phillips, B.A., Allen, D.A.: 1979, Mon. Not. R. astr. Soc. 187, 813 Google Scholar
Feast, M.W., Robertson, B.R.C., Catchpole, R.: 1977, Mon. Not. R. astr. Soc. 179, 499 Google Scholar