Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T04:49:22.957Z Has data issue: false hasContentIssue false
  • English
  • Français

JHK Observations of Magellanic Cloud Cepheids

Published online by Cambridge University Press:  04 August 2017

D. L. Welch  and
B. F. Madore
D. L. Welch
Affiliation:
Department of Astronomy, David Dunlap Observatory, University of Toronto, Toronto, Ontario, Canada M5S 1A1
B. F. Madore
Affiliation:
Department of Astronomy, David Dunlap Observatory, University of Toronto, Toronto, Ontario, Canada M5S 1A1

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.

The pioneering work of McGonegal et al. (1982), originally employing random-phase data for the LMC near-infrared period-luminosity (P-L) relation, is refined to mean light and extended to the SMC using new observations. We use a procedure for reducing single-phase infrared observations to mean light to obtain JHK magnitudes for Magellanic Cloud Cepheids. The new <H> P-L relations are presented and discussed.

Type
Stellar Populations
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 221 - 222
Copyright
Copyright © Reidel 1984 

References

McGonegal, R., McLaren, R.A., McAlary, C.W., and Madore, B.F. 1982, Astrophys. J. (Letters), L33.Google Scholar
Payne-Gaposchkin, C. and Gaposchkin, S. 1966, Smithson. Contr. Astrophys. 9.CrossRefGoogle Scholar
Welch, D.L., Wieland, F., McAlary, C.W., McGonegal, R., Madore, B.F., McLaren, R.A., and Neugebauer, G. 1984, Astrophys. J. Suppl. (submitted).Google Scholar