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astro-ph.SRastro-ph.HEastro-ph.GAastro-phastro-ph.IMgr-qcastro-ph.EPastro-ph.COphysics.data-anphysics.flu-dyn

On Valency

published · living versions
W_64q97rmd·v1 · currentpublished
A high fraction of close massive binary stars at low metallicity
with H. Sana, T. Shenar, J. Bodensteiner, N. Britavskiy +72
1 version

Preprints & journals

102 papers in the corpus · 2005–2026
You're Gonna Need a Bigger Core: Calibrating Massive Star Models against Galactic OB-type Stars2608.02540v1 · Thibault Lechien, Selma E. de Mink, Stephen Justham et al.2026 · 0 citationsarXiv
Thermal-timescale accretion does not always yield critical rotation in mass gainers2601.08508v1 · Chen Wang, Mike Y.M. Lau, Xiang-Dong Li et al.2026 · 4 citationsarXiv
Dynamical binary interactions in the 2040s2512.14802v1 · Nadejda Blagorodnova, Ondrej Pejcha, Tomek Kami'nski et al.2025 · 0 citationsarXiv
He-star donor pathway for the hypervelocity star D6-22511.11998v1 · Abinaya Swaruba Rajamuthukumar, Ruediger Pakmor, Stephen Justham et al.2025 · 0 citationsarXiv
Violent mergers revisited: The origin of the fastest stars in the Galaxy2510.11781v2 · Rudiger Pakmor, Ken J. Shen, Aakash Bhat et al.2025 · 1 citationarXiv
A high fraction of close massive binary stars at low metallicity2509.12488v1 · H. Sana, T. Shenar, J. Bodensteiner et al.2025 · 26 citationsNature Astronomy (2025)on Valency
Good things come to those who wait: Watching donor stars evolve towards a mass-transfer instability2509.09492v1 · Karel D. Temmink, Onno R. Pols, Stephen Justham et al.2025 · 4 citationsA&A 703, A121 (2025)
A half-ring of ionized circumstellar material trapped in the magnetosphere of a white dwarf merger remnant2507.13850v1 · Andrei A. Cristea, Ilaria Caiazzo, Tim Cunningham et al.2025 · 4 citationsarXiv
Binary mass transfer in 3D: Mass Transfer Rate and Morphology2505.18255v4 · T. Ryu, R. Sari, S. E. de Mink et al.2025 · 9 citationsA&A 702, A61 (2025)
Evidence of polar and ultralow supernova kicks from the orbits of Be X-ray binaries2505.08857v1 · Ruggero Valli, Selma E. de Mink, Stephen Justham et al.2025 · 5 citationsarXiv
The ii-processes nucleosynthesis during the formation of He-rich hot-subdwarf stars2503.23541v1 · T. Battich, M. M. Miller Bertolami, A. Weiss et al.2025 · 4 citationsA&A 699, A298 (2025)
Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors2503.00115v2 · Aldana Grichener, Mathieu Renzo, Wolfgang E. Kerzendorf et al.2025 · 6 citationsarXiv
The role of triple evolution in the formation of LISA double white dwarfs2502.09607v2 · Abinaya Swaruba Rajamuthukumar, Valeriya Korol, Jakob Stegmann et al.2025 · 6 citationsA&A 704, A156 (2025)
Planet formation and long-term stability in a very eccentric stellar binary2501.05506v1 · Jakob Stegmann, Evgeni Grishin, Cole Johnston et al.2025 · 0 citationsarXiv
Large-scale ordered magnetic fields generated in mergers of helium white dwarfs2407.02566v2 · Rudiger Pakmor, Ingrid Pelisoli, Stephen Justham et al.2024 · 17 citationsA&A 691, A179 (2024)
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Convection in 3D Simulations of Red Supergiants2311.16885v2 · Jing-Ze Ma, Andrea Chiavassa, Selma E. de Mink et al.2023 · 24 citationsApJL 962 L36 (2024)
A self-synthesized origin of heavy metals in hot subdwarf stars?2311.04700v1 · T. Battich, M. M. Miller Bertolami, A. M. Serenelli et al.2023 · 0 citationsarXiv
The Potential of Asteroseismology to Resolve the Blue Supergiant Problem2311.00038v2 · Earl Patrick Bellinger, Selma E. de Mink, Walter E. van Rossem et al.2023 · 25 citationsarXiv
The bright blue side of the night sky: Spectroscopic survey of bright and hot (pre-) white dwarfs2307.03721v1 · Nicole Reindl, Ramazan Islami, Klaus Werner et al.2023 · 21 citationsA&A 677, A29 (2023)
Observational predictions for Thorne-Żytkow objects2305.07337v2 · R. Farmer, M. Renzo, Y. Gotberg et al.2023 · 19 citationsarXiv
Nucleosynthesis of binary-stripped stars2303.04520v1 · R. Farmer, E. Laplace, Jing-ze Ma et al.2023 · 42 citationsarXiv
The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters2211.15794v2 · Chen Wang, Ben Hastings, Abel Schootemeijer et al.2022 · 24 citationsA&A 670, A43 (2023)
Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators2211.01564v1 · H.Xiong, L.Casagrande, X.Chen et al.2022 · 20 citationsA&A 668, A112 (2022)
Coping with loss: Stability of mass transfer from post-main sequence donor stars2209.12707v3 · K. D. Temmink, O. R. Pols, S. Justham et al.2022 · 0 citationsA&A 669, A45 (2023)
The circumstellar material around the Type IIP SN 2021yja2207.09976v2 · Alexandra Kozyreva, Jakub Klencki, Alexei V. Filippenko et al.2022 · 20 citationsarXiv
Discovery of a highly magnetic He-sdO star from a double-degenerate binary merger2201.08146v2 · M. Dorsch, N. Reindl, I. Pelisoli et al.2022 · 21 citationsA&A 658, L9 (2022)
The Next Generation Global Gravitational Wave Observatory: The Science Book2111.06990v1 · Vicky Kalogera, B.S. Sathyaprakash, Matthew Bailes et al.2021 · 34 citationsarXiv
The cosmic carbon footprint of massive stars stripped in binary systems2110.04131v2 · R. Farmer, E. Laplace, S.E. de Mink et al.2021 · 33 citationsarXiv
The redshift evolution of the binary black hole merger rate: a weighty matter2110.01634v2 · L. A. C. van Son, S. E. de Mink, T. Callister et al.2021 · 148 citationsThe Astrophysical Journal, Volume 931, (2022) 17
Rapid stellar and binary population synthesis with COMPAS2109.10352v3 · Team COMPAS: Jeff Riley, Poojan Agrawal, Jim W. Barrett et al.2021 · 158 citationsarXiv
Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers2103.02608v3 · Floor S. Broekgaarden, Edo Berger, Coenraad J. Neijssel et al.2021 · 151 citationsarXiv
Different to the core: the pre-supernova structures of massive single and binary-stripped stars2102.05036v2 · E. Laplace, S. Justham, M. Renzo et al.2021 · 159 citationsA&A 656, A58 (2021)
Career total: 207 works. 102 are in this corpus.Showing the 50 most recent.

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