Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-19T18:17:50.485Z Has data issue: false hasContentIssue false
  • English
  • Français

AR Pavonis: the Rosetta stone of the symbiotics

Published online by Cambridge University Press:  12 April 2016

Mark H. Slovak
Mark H. Slovak*
Affiliation:
University of Texas at Austin, USA

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.

With Mayall’s discovery of the eclipsing nature of AR Pavonis = CD-66°3307, a nearby unique opportunity to directly probe the structure of the symbiotic binary became available. Few eclipsing systems have been detected among the symbiotics and AR Pav is fortunately bright enough to be observed spectroscopically at Coudé dispersions.

Type
Session II – Discussion on Individual Stars
Information
International Astronomical Union Colloquium , Volume 70: The Nature of Symbiotic Stars , 1982 , pp. 195 - 200
Copyright
Copyright © Reidel 1982

References

Allen, D.A.: 1978, in IAU Coll. No.45, “Changing Trends in Variable Star Research”, Hamilton, New Zeeland, p.125.Google Scholar
Andrews, P.J.: 1974, Mon.Not.R.astr. Soc. 167, 635 Google Scholar
Glass, I.S., and Webster, B.L.: 1973, Mon.Not.R.astr.Soc. 165, 77. Google Scholar
Mayall, M.W.: 1937, Harvard Annals 105, 491. Google Scholar
Sahade, J.: 1949, Astrophys.J. 109, 541.Google Scholar
Slovak, M.H.: 1981, Unpublished PhD Thesis, University of Texas. Google Scholar
Thackeray, A.D.: 1959, Mon.Not.R.astr.Soc. 119, 629.Google Scholar
Thackeray, A.D., and Hutchings, J.B.: 1974, Mon. Not.R.astr.Soc. 167, 319. Google Scholar
Wright, A.E., and Allen, D.A.: 1978, Mon.Not.R.astr.Soc. 184, 893.CrossRefGoogle Scholar