Calibrating the Cepheid Period-Luminosity relation with the VLTI

M. Marengo; M. Karovska; D. Sasselov; C. Papaliolios; J. T. Armstrong; T. E. Nordgren

doi:10.1051/eas:2003026

All issues

Volume 6 (2003)

EAS Publications Series, 6 (2003) 265

Abstract

Issue		EAS Publications Series Volume 6, 2003 Observing with the VLTI


Page(s)		265 - 265
DOI		https://doi.org/10.1051/eas:2003026
Published online		31 January 2003

Observing with the VLTI
G. Perrin and F. Malbet (eds)
EAS Publications Series, 6 (2003) 265

Calibrating the Cepheid Period-Luminosity relation with the VLTI

M. Marengo¹, M. Karovska¹, D. Sasselov¹, C. Papaliolios¹, J. T. Armstrong² and T. E. Nordgren³

¹ Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
² Naval Research Laboratory, Code 7210, Washington, DC 20375, USA
³ University of Redlands, 1200 E Colton Ave, Redlands, CA, USA

Abstract

The VLTI is the ideal instrument for measuring the distances of nearby Cepheids with the Baade-Wesselink method, allowing an accurate recalibration of the Cepheid Period-Luminosity relation. The high accuracy required by such measurement, however, can only be reached taking into account the effects of limb darkening, and its dependence on the Cepheid pulsations. We present here our new method to compute phase- and wavelength-dependent limb darkening profiles, based on hydrodynamic simulation of Classical Cepheid atmospheres.