The Components of Cepheid Systems: The FN Vel System*

Abstract Cepheid masses continue to be important tests of evolutionary tracks for intermediate-mass stars as well as important predictors of their future fate. For systems where the secondary is a B star, Hubble Space Telescope ultraviolet spectra have been obtained. From these spectra a temperature can be derived, and from this a mass of the companion M 2 . Once Gaia DR4 is available, proper motions can be used to determine the inclination of the orbit. Combining mass of the companion, M 2 , the mass function from the ground-based orbit of the Cepheid and the inclination produces the mass of the Cepheid, M 1 . The Cepheid system FN Vel is used here to demonstrate this approach and what limits can be put on the Cepheid mass for inclination between 50° and 130°.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2024-10-24
DOI
https://doi.org/10.3847/1538-3881/ad7fea
Citations
3
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.99

Funders

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article

The Components of Cepheid Systems: The FN Vel System*

Charles Proffitt, Richard I. Anderson, Joanna Kuraszkiewicz, Hans Moritz Günther et al.
3 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
0.99
article

The Components of Cepheid Systems: The FN Vel System*

Charles Proffitt, Richard I. Anderson, Joanna Kuraszkiewicz, Hans Moritz Günther, Boris Trahin, A. Mérand, Nancy Remage Evans, A. Gallenne, P. Kervella, Giordano Viviani, Shreeya Shetye
article en
3 citations

Abstract

Abstract Cepheid masses continue to be important tests of evolutionary tracks for intermediate-mass stars as well as important predictors of their future fate. For systems where the secondary is a B star, Hubble Space Telescope ultraviolet spectra have been obtained. From these spectra a temperature can be derived, and from this a mass of the companion M 2 . Once Gaia DR4 is available, proper motions can be used to determine the inclination of the orbit. Combining mass of the companion, M 2 , the mass function from the ground-based orbit of the Cepheid and the inclination produces the mass of the Cepheid, M 1 . The Cepheid system FN Vel is used here to demonstrate this approach and what limits can be put on the Cepheid mass for inclination between 50° and 130°.

The Astronomical JournalVol. 168(5)
National Aeronautics and Space Administration, Space Telescope Science Institute, European Space Agency, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Vlaamse regering, Agencia Nacional de Investigación y Desarrollo, European Research Council, Astrophysics Division, Fondo Nacional de Desarrollo Científico y Tecnológico, HORIZON EUROPE European Research Council
Openalex Percentile: Top 23%
Stellar, planetary, and galactic studies
0.99
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The Components of Cepheid Systems: The FN Vel System* — Charles Proffitt, Richard I. Anderson, et al. · The Astronomical Journal (2024) | TGRS Research Map | TGRS