Revisiting bright delta Scuti stars and their period-luminosity relation with TESS and Gaia DR3
arXiv:2207.00343 · doi:10.1093/mnras/stac2132
Abstract
We have used NASA's TESS mission to study catalogued delta Scuti stars. We examined TESS light curves for 434 stars, including many for which few previous observations exist. We found that 62 are not delta Scuti pulsators, with most instead showing variability from binarity. For the 372 delta Scuti stars, we provide a catalogue of the period and amplitude of the dominant pulsation mode. Using Gaia DR3 parallaxes, we place the stars in the period-luminosity diagram and confirm previous findings that most stars lie on a ridge that corresponds to pulsation in the fundamental radial mode, and that many others fall on a second ridge that is a factor two shorter in period. This second ridge is seen more clearly than before, thanks to the revised periods and distances. We demonstrate the value of the period-luminosity diagram in distinguishing delta Scuti stars from short-period RR Lyrae stars, and we find several new examples of high-frequency delta Scuti stars with regular sequences of overtone modes, including XX Pyx and 29 Cyg. Finally, we revisit the sample of delta Scuti stars observed by Kepler and show that they follow a tight period-density relation, with a pulsation constant for the fundamental mode of Q = 0.0315 d.
arXiv commentpublished by MNRAS
References in corpus (22)
- dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
- The VizieR database of Astronomical Catalogues
- Probing the interior physics of stars through asteroseismology
- Asteroseismology of red giants from the first four months of Kepler data: Global oscillation parameters for 800 stars
- {\em Gaia}-derived luminosities of {\em Kepler} A/F stars and the pulsator fraction across the δ Scuti instability strip
- Amplitude modulation in Sct stars: statistics from an ensemble study of Kepler targets
- Very regular high-frequency pulsation modes in young intermediate-mass stars
- Catalogue and Properties of δ Scuti Stars in Binaries
- An examination of some characteristics of Kepler Short and Long Cadence Data
- Gravity-mode period spacings and near-core rotation rates of 611 Doradus stars with \textit{Kepler}
- The period-luminosity relation for delta Scuti stars using Gaia DR2 parallaxes
- The ASAS-SN Catalog of Variable Stars VI: An All-Sky Sample of Scuti Stars
- Statistical Properties of Galactic δ Scuti Stars: Revisited
- First results on RR Lyrae stars with the TESS space telescope: untangling the connections between mode content, colors and distances
- Highlights of Discoveries for Scuti Variable Stars From the Kepler Era
- Tidally perturbed pulsations in the pre-main sequence Scuti binary RS Cha
- Five young Scuti stars in the Pleiades seen with Kepler/K2
- Observational and Theoretical Studies of 27 Scuti Stars with Investigation of the Period-Luminosity Relation
- The Pulsation Properties of Bootis Stars I. The Southern TESS Sample
- Beta Cephei stars in the ASAS-3 data. I. Long-term variations of periods and amplitudes
- Convection and Overshoot in models of gamma Doradus and delta Scuti stars
- Metal-Rich RRc stars in the Carnegie RR Lyrae Survey
Cited by in corpus (13)
- Asteroseismology of Scuti stars: emulating model grids using a neural network
- Identifying 850 delta Scuti pulsators in a narrow Gaia colour range with TESS 10-minute full-frame images
- A segmented period-luminosity relation for nearby extragalactic Scuti stars
- TESS Observations of Seven Newly Identified High-amplitude Scuti Stars
- Period-Colour and Amplitude-Colour relations for OGLE- Scuti stars in the Galactic Bulge and LMC
- Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for SX Phoenicis Variables in the gri-Band
- Short-Period Variables in TESS Full-Frame Image Light Curves Identified via Convolutional Neural Networks
- Modelling Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
- Exploring the convective core of the high-amplitude Scuti star TIC 120857354 with asteroseismology
- The extraordinary frequency pattern variation in δ Scuti stars
- Characterizing bright Scuti pulsators using TESS lightcurves
- Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS
- Investigating the Period-Luminosity Relations of delta Scuti Stars: A Pathway to Distance and 3-D Dust Map Inference