Hostname: page-component-5c6d5d7d68-qks25 Total loading time: 0 Render date: 2024-08-21T07:13:37.866Z Has data issue: false hasContentIssue false
  • English
  • Français

Recent Results on Cepheids in the Magellanic Clouds from the EROS Survey

Published online by Cambridge University Press:  25 May 2016

J.B. Marquette
J.B. Marquette*
Affiliation:
Institut d'Astrophysique de Paris, 98bis Bd Arago, 75014 Paris, France

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.

Between October 1996 and February 1997 a specific campaign of the EROS experiment was devoted to Cepheids in central regions of the LMC and the SMC. The Period–Luminosity (PL) relations were determined in the EROS photometric system, and a significant slope change of the period–luminosity relation has been observed for the SMC fundamental mode Cepheids with periods shorter than 2 days.

Type
Part 8. Cepheids and Distances
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 523 - 526
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Ansari, R. 1996, Vistas in Astronomy, 40, 519 Google Scholar
Bauer, F. 1997, , Google Scholar
Bauer, F., et al. (the EROS coll.) 1997, in Optical Detectors for Astronomy, ESO: Garching Google Scholar
Bauer, F., et al. (the EROS coll.) 1999, in preparation Google Scholar
Beaulieu, J.P., et al. (the EROS coll.) 1995, ApJ, 303, 137 Google Scholar
Beaulieu, J.P., & Sasselov, D. (the EROS coll.) 1996, in Variable Stars and the Astrophysical Returns of Microlensing Surveys, Ferlet, R., Maillard, J.P., & Raban, B., Frontières: Paris, 1996, 193 Google Scholar
Scargle, J.D. 1982, ApJ, 263, 835 Google Scholar