Image de couverture de livre

Power density spectra morphologies of seismically unresolved red-giant asteroseismic binaries

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Choi, Jeong Yun, Espinoza-Rojas, Francisca, Coppée, Quentin, Hekker, Saskia
Format:	Preprint
Publié:	2025
Sujets:	Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Hidden oscillations in plain sight: identification of seismically unresolved red-giant asteroseismic binary candidates
par: Choi, Jeong Yun, et autres
Publié: (2026)

Red giant asteroseismic binaries in the Kepler field
par: Espinoza-Rojas, Francisca, et autres
Publié: (2025)

Oscillations of red giant stars with magnetic damping in the core. I. Dissipation of mode energy in dipole-like magnetic fields
par: Müller, Jonas, et autres
Publié: (2025)

The radial modes of stars with suppressed dipole modes
par: Coppée, Quentin, et autres
Publié: (2024)

Asymptotic power spectra and visibilities of damped mixed modes
par: Müller, Jonas, et autres
Publié: (2026)

The efficiency of mixed modes for angular momentum transport
par: Bordadágua, Beatriz, et autres
Publié: (2025)

Ensemble seismic study of the properties of the core of Red Clump stars
par: Noll, Anthony, et autres
Publié: (2025)

Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants
par: Larsen, Jens R., et autres
Publié: (2025)

Weak or strong: coupling of mixed oscillation modes on the red-giant branch
par: van Lier, T., et autres
Publié: (2025)

The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
par: Hekker, S., et autres
Publié: (2026)

Effect of nuclear reactions rates and core boundary mixing on the seismology of red clump stars
par: Noll, Anthony, et autres
Publié: (2024)

Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars
par: van Lier, T., et autres
Publié: (2026)

The highest mass Kepler red giants -- I. Global asteroseismic parameters of 48 stars
par: Crawford, Courtney L., et autres
Publié: (2024)

The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
par: Ahlborn, F., et autres
Publié: (2024)

Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages
par: Vitali, S., et autres
Publié: (2024)

Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
par: Ahlborn, F., et autres
Publié: (2025)

DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations
par: Mazzi, A., et autres
Publié: (2025)

Surface brightness-color relations for red giant branch stars using asteroseismic radii and Gaia distances (the ARD method)
par: Xiong, Jianping, et autres
Publié: (2025)

The role of stellar model input in correcting the asteroseismic scaling relations. Red giant branch models
par: Valle, G., et autres
Publié: (2025)

Linearity of Structure Kernels in Main-sequence and Subgiant Solar-like Oscillators
par: Buchele, Lynn, et autres
Publié: (2025)

Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
par: Buchele, Lynn, et autres
Publié: (2024)

Testing the asteroseismic estimates of stellar radii with surface brightness-colour relations and Gaia DR3 parallaxes. Red giants and red clump stars
par: Valle, G., et autres
Publié: (2024)

Merger seismology: distinguishing massive merger products from genuine single stars using asteroseismology
par: Henneco, Jan, et autres
Publié: (2024)

Understanding post-red giant branch binaries through stable mass transfer
par: Moltzer, C. A. S., et autres
Publié: (2025)

A comprehensive Gaia view of ellipsoidal and rotational red giant binaries
par: Navarrete, Camila, et autres
Publié: (2025)

Testing tidal theory using Gaia binaries: the red giant branch
par: Dewberry, Janosz W., et autres
Publié: (2025)

Improving the stellar age determination through joint modeling of binarity and asteroseismology -- Grid modeling of the seismic red-giant binary KIC 9163796
par: Grossmann, D. H., et autres
Publié: (2025)

Testing the asteroseismic estimates of stellar radii with surface brightness-colour relations and {\it Gaia} DR3 parallaxes. II. Red giants and red clump stars from the {\it Kepler} catalogue
par: Valle, G., et autres
Publié: (2024)

Unequivocal detection of the tidal deformation of a red giant in a binary system via interferometry
par: Merc, Jaroslav, et autres
Publié: (2024)

Li-enrichment in red clump giants: Clues for past binary interaction or merger events
par: Singh, Raghubar, et autres
Publié: (2025)

Asteroseismic Inversions for Internal Sound Speed Profiles of Main-sequence Stars with Radiative Cores
par: Buchele, Lynn, et autres
Publié: (2023)

Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
par: Thomsen, J. S., et autres
Publié: (2025)

Enhanced magnetic activity in rapidly rotating binary stars
par: Yu, Jie, et autres
Publié: (2025)

A population synthesis study of the Gaia 100 pc unresolved white dwarf-main sequence binary population
par: Santos-García, Alejandro, et autres
Publié: (2025)

A magnitude-limited catalogue of unresolved white dwarf-main sequence binaries from Gaia DR3
par: Rebassa-Mansergas, Alberto, et autres
Publié: (2025)

An improved asteroseismic age of the rapid rotator Altair from TESS data
par: Rieutord, Michel, et autres
Publié: (2024)

Modeling APOKASC-3 red giants: I. The first dredge-up and red giant branch bump
par: Cao, Kaili, et autres
Publié: (2025)

Homogenous abundances of Mg, Si, Ca, and Ti for about 1500 red giants in 16 globular clusters from FLAMES spectra
par: Carretta, Eugenio
Publié: (2026)

Anomalously fast core and envelope rotation in red giants
par: Dhanpal, Siddharth, et autres
Publié: (2025)

Near-critical magnetic fields in Kepler red giants
par: Deheuvels, S., et autres
Publié: (2026)