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20122026
most citedPulsating red giant stars in eccentric binary systems discovered from Kepler space-based photometry

137 citations · 1.1k across the 35 of their papers we have counts for

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34 papers · 1 filter

astro-ph.SR2026★ 2 cited

Wide sdB binaries. I. Orbital and atmospheric parameters

Francisco Molina, Joris Vos, Alexey Bobrick +1

Long-period binary systems containing a B-type hot subdwarf (sdB) and a main-sequence companion are thought to originate from binary interactions involving stable mass transfer fro…

astro-ph.SR2023

The mass range of hot subdwarf B stars from MESA simulations

Eduardo Arancibia-Rojas, Monica Zorotovic, Maja Vučković +3

Hot subdwarf B (sdB) stars are helium core burning stars that have lost almost their entire hydrogen envelope due to binary interaction. Their assumed canonical mass of $\rm M_{\ma…

astro-ph.SR2023★ 25 cited

MELCHIORS: The Mercator Library of High Resolution Stellar Spectroscopy

P. Royer, T. Merle, K. Dsilva +71

Over the past decades, libraries of stellar spectra have been used in a large variety of science cases, including as sources of reference spectra for a given object or a given spec…

astro-ph.SR2022★ 30 cited

Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra

Zhenxin Lei, Ruijie He, Peter Nemeth +6

222 hot subdwarf stars were identified with LAMOST DR8 spectra, among which 131 stars show composite spectra and have been decomposed, while 91 stars present single-lined spectra.…

astro-ph.SR2022★ 21 cited

Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators

H. Xiong, L. Casagrande, X. Chen +7

Blue large-amplitude pulsators (BLAPs) are a newly discovered type of variable star. Their typical pulsation periods are on the order of a few tens of minutes, with relatively larg…

astro-ph.SR2022★ 3 cited

Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars I. Sample selection and binary classification method

Murat Uzundag, Matias I. Jones, Maja Vučković +3

The current theory predicts that hot subdwarf binaries are produced from evolved low-mass binaries that have undergone mass transfer and drastic mass loss during either a common en…