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Cited article:

A Novel q-PED Method: Precise Physical Properties of a Merger-origin Binary Cepheid OGLE-LMC-CEP-1347

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Exploring the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth

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Non-evolutionary effects on period change in Magellanic Cepheids

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Synthetic Population of Binary Cepheids. II. The Effect of Companion Light on the Extragalactic Distance Scale

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Orbit determination for the binary Cepheid V1344 Aql

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Synthetic Population of Binary Cepheids. I. The Effect of Metallicity and Initial Parameter Distribution on Characteristics of Cepheids’ Companions

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Discovery of a Binary-origin Classical Cepheid in a Binary System with a 59 day Orbital Period* †

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The η Aquilae System: Radial Velocities and Astrometry in Search of η Aql B

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Multiplicity of Galactic Cepheids and RR Lyrae stars from Gaia DR2

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The occurrence of binary evolution pulsators in classical instability strip of RR Lyrae and Cepheid variables

P. Karczmarek, G. Wiktorowicz, K. Iłkiewicz, et al.
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PROPERTIES OF THE OPEN CLUSTER TOMBAUGH 1 FROM HIGH-RESOLUTION SPECTROSCOPY AND uvbyCaHβ PHOTOMETRY*

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VETTING GALACTIC LEAVITT LAW CALIBRATORS USING RADIAL VELOCITIES: ON THE VARIABILITY, BINARITY, AND POSSIBLE PARALLAX ERROR OF 19 LONG-PERIOD CEPHEIDS

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THE ARAUCARIA PROJECT: A STUDY OF THE CLASSICAL CEPHEID IN THE ECLIPSING BINARY SYSTEM OGLE LMC562.05.9009 IN THE LARGE MAGELLANIC CLOUD

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The strange evolution of the Large Magellanic Cloud Cepheid OGLE-LMC-CEP1812

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