Constructing a Cepheid Period p-Factor Relation from Static Model Stellar Atmospheres

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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2 pages, 1 figure, To be published in Astrophysics and Space Science Proceedings series (ASSP). Proceedings of the "20th Stell

Scientific paper

One of the largest uncertainties for using the Baade-Wesselink method to
measure Cepheid distances is the value of the projection factor (p-factor).
However, p-factors measured using the IRSB technique and from hydrodynamic
models disagree. In this work, we compute spherically-symmetric static model
stellar atmospheres and predict a period p-factor relation.

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