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20182026
most citedLow-frequency gravity waves in blue supergiants revealed by high-precision space photometry

165 citations · 649 across the 15 of their papers we have counts for

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astro-ph.SR2026

Wildly Oscillating Stars -- Unexplained dense ridge-like frequency agglomerations in A and F type pulsators

V. Antoci, J. Labadie-Bartz, M. Swiech +14

We investigate the origin of the dense, ridge-like frequency clusters observed in a subset of A and F type pulsating stars, which we refer to as `wildly oscillating' stars (WOS). T…

astro-ph.SR2025

Beyond prewhitening: detection of gravity modes and their period spacings in slowly pulsating B stars using the multitaper F-test

Aarya A. Patil, Conny Aerts, Nikki Y. N. Wang +2

Gravity modes in main-sequence stars have traditionally been studied using a prewhitening approach, which iteratively identifies modes in the Fourier domain and subsequently tunes…

astro-ph.SR20245 cited

MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators

N. Jannsen, A. Tkachenko, P. Royer +14

With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's poten…

astro-ph.SR2023

X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

Jorick S. Vink, A. Mehner, P. A. Crowther +78

Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational-wave events involving spectacular black-hole mergers, indicate that the low…

astro-ph.SR202340 cited

Convective boundary mixing in main-sequence stars: theory and empirical constraints

Evan H. Anders, May G. Pedersen

The convective envelopes of solar-type stars and the convective cores of intermediate- and high-mass stars share boundaries with stable radiative zones. Through a host of processes…

astro-ph.SR202322 cited

Contamination in TESS light curves: The case of the Fast Yellow Pulsating Supergiants

May G. Pedersen, Keaton J. Bell

Given its large plate scale of 21" / pixel, analyses of data from the TESS space telescope must be wary of source confusion from blended light curves, which creates the potential t…