Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-13T10:46:20.498Z Has data issue: false hasContentIssue false
  • English
  • Français

Another Look at the RV Tauri Period-Luminosity Relation

Published online by Cambridge University Press:  12 April 2016

Glenn M. Wahlgren
Glenn M. Wahlgren*
Affiliation:
Astronomy Programs, Computer Sciences Corporation, Space Telescope Science Institute

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.

The Period-Luminosity (P-L) relation for the RV Tauri variables (DuPuy 1973) contradicts those of other variables in the instability strip as it predicts lower luminosity at longer pulsational periods. It is based primarily upon three globular cluster variables. DuPuy determined secular and statistical parallaxes from 23 field variables, defining a simple P-L relation with a slightly negative slope.

Type
4. The Variability-Evolution Connection
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 295
Copyright
Copyright © Cambridge University Press 1989

References

Dupuy, D.L. 1973. Ap. J. 185, 597.Google Scholar
Gingold, R.A. 1976. Ap. J. 204, 116.Google Scholar
Takeuti, M. and Petersen, J.O. 1983, Astron. Astrophvs. 117, 352.Google Scholar
Wahlgren, G.M. 1986, Ph.D. Thesis. The Ohio State University.Google Scholar