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High resolution spectroscopy for Cepheids distancedetermination

2006/06/09 by N. Nardetto, D. Mourard, P. Kervella +5 · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics and Star Formation Studies #High-pressure geophysics and materials #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20054333

published as Astron.Astrophys.453:309,2006

openalex publication_date 2006/06/09 · arxiv created 2008/04/08 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context.The ratio of pulsation to radial velocity (the projection factor) is currently limiting the accuracy of the Baade-Wesselink method, and in particular of its interferometric version recently applied to several nearby Cepheids.

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