collaborators

7 papers

astro-ph.SR2025

VELOCE III. Reconstructing Radial Velocity Curves of Classical Cepheids

Giordano Viviani, Richard I. Anderson

We present a novel framework for accurately reconstructing radial velocity (RV) curves of classical Cepheids (Cepheids) from sparsely sampled time-series data suitable for applicat…

astro-ph.SR2025

A joint 1% calibration of the RR Lyrae & type-II Cepheid Leavitt laws yields homogeneous distances to 93 Galactic globular clusters

Bastian Lengen, Richard I. Anderson, Mauricio Cruz Reyes +1

Recent work has established large samples of astrometrically confirmed RR Lyrae and type-II Cepheid members of Galactic globular clusters (GCs). Any given GC can contain multiple s…

astro-ph.SR2025

V659 Cen: System Parameters Updated

Nancy Remage Evans, Charles Proffitt, Pierre Kervella +8

V659 Cen is a classical Cepheid which is part of a multiple system. Previous observations have shown that a hot companion dominates an ultraviolet spectrum and a cooler main sequen…

astro-ph.SR2025

Mass of Cepheid V350 Sgr Incorporating Interferometry and the Companion Mass

Nancy Remage Evans, Alexandre Gallenne, Pierre Kervella +8

The system V350 Sgr has a classical Cepheid for the primary. Interferometry is presented for the system and the full orbit is determined. The mass of the companion has been determi…

astro-ph.SR2025

The VELOCE modulation zoo III. Detecting additional pulsation modes in optical spectra of classical Cepheids using semi-partial distance correlation periodograms

Kent Barbey, Richard Irving Anderson, Giordano Viviani +5

Known for their large amplitude radial pulsations, classical Cepheids are critical standard candles in astrophysics. However, they also exhibit various pulsational irregularities a…

astro-ph.SR2024

The VELOCE modulation zoo II. Humps and splitting patterns in spectral lines of classical Cepheids

H. Netzel, R. I. Anderson, G. Viviani

Line splitting in spectral lines is observed in various types of stars due to phenomena such as shocks, spectroscopic binaries, magnetic fields, spots, and non-radial modes. In pul…