Recent interferometric observations of the brightest and angularly largest classical Cepheid, l Carinae, with ESO's Very Large Telescope Interferometer have resolved with high precision the variation of its angular diameter with phase. We compare the measured angular diameter curve to the one that we derive by an application of the...
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April 2004 (v1)Journal articleUploaded on: December 4, 2022
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March 1, 2017 (v1)Journal article
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October 17, 2024 (v1)Journal article
Context. The Baade-Wesselink (BW) method, also known as the pulsation parallax method, allows us to estimate distances to individual pulsating stars. Accurate geometric parallaxes obtained by the Gaia mission serve us in the calibration of the method and in the determination of its precision. This method also provides a way of determining mean...
Uploaded on: January 13, 2025 -
November 2020 (v1)Journal article
Aims. Classical Cepheids provide the foundation for the empirical extragalactic distance ladder. Milky Way Cepheids are the only stars in this class accessible to trigonometric parallax measurements. However, the parallaxes of Cepheids from the second Gaia data release (GDR2) are affected by systematics because of the absence of chromaticity...
Uploaded on: December 4, 2022 -
July 8, 2020 (v1)Publication
Classical Cepheids provide the foundation for the empirical extragalactic distance ladder. Milky Way Cepheids are the only stars in this class accessible to trigonometric parallax measurements. However, the parallaxes of Cepheids from the second Gaia data release (GDR2) are affected by systematics because of the absence of chromaticity...
Uploaded on: February 22, 2023 -
January 8, 2020 (v1)Publication
Classical Cepheids (CCs) are at the heart of the empirical extragalactic distance ladder. Milky Way CCs are the only stars of this class accessible to trigonometric parallax measurements. Until recently, the most accurate trigonometric parallaxes of Milky Way CCs were the HST/FGS measurements collected by Benedict et al. (2002, 2007)....
Uploaded on: December 4, 2022 -
July 8, 2020 (v1)Publication
Classical Cepheids provide the foundation for the empirical extragalactic distance ladder. Milky Way Cepheids are the only stars in this class accessible to trigonometric parallax measurements. However, the parallaxes of Cepheids from the second Gaia data release (GDR2) are affected by systematics because of the absence of chromaticity...
Uploaded on: December 4, 2022 -
2017 (v1)Journal article
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July 20, 2018 (v1)Journal article
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November 1, 2020 (v1)Journal article
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February 10, 2019 (v1)Journal article
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Uploaded on: December 4, 2022