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Mass and p-factor of the Type II Cepheid OGLE-LMC-T2CEP-098 in a Binary System

  • Authors: Bogumił Pilecki, Wolfgang Gieren, Radosław Smolec, Grzegorz Pietrzyński, Ian B. Thompson, Richard I. Anderson, Giuseppe Bono, Igor Soszyński, Pierre Kervella, Nicolas Nardetto, Mónica Taormina, Kazimierz Stȩpień, and Piotr Wielgórski

2017 The Astrophysical Journal 842 110.

  • Provider: AAS Journals

Caption: Figure 9.

Pulsational radial velocity curve (points) and the radius variation (solid lines) of the Cepheid over one pulsation cycle. To obtain this RV curve the orbital motion was removed from the measured radial velocities. The full range of ﹩{\rm{\Delta }}R﹩ is ﹩5.7\mbox{--}6.7\,{R}_{\odot }﹩, depending on the assumed p-factor (1.2–1.4).

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