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Testing red clump models with the asteroseismic binary KIC 10841730
Lea S Schimak, Timothy R Bedding, Courtney L Crawford, Paul G Beck, Yaguang Li, Daniel Huber, Joel Ong, Benjamin T Montet, May Gade Pedersen, Desmond H Grossmann, Savita Mathur and Rafael A García Monthly Notices of the Royal Astronomical Society 546(3) (2026) https://doi.org/10.1093/mnras/stag151
Not all nitrogen-rich field stars originate from globular clusters
E. I. Leitinger, A. Miglio, J. Montalbán, D. Massari, A. Bragaglia, W. E. van Rossem, K. Brogaard, A. Mazzi, J. S. Thomsen and E. Willett Astronomy & Astrophysics 708 A346 (2026) https://doi.org/10.1051/0004-6361/202558003
A Plasmoid Model for Mass Loss from Stars on the Upper Red Giant Branch: The Mass-loss Rate is Controlled by the Number of Density Scale Heights in the Convection Zone
DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations
A. Mazzi, J. S. Thomsen, A. Miglio, K. Brogaard, L. Girardi, D. Bossini, M. Matteuzzi and W. E. van Rossem Astronomy & Astrophysics 699 A39 (2025) https://doi.org/10.1051/0004-6361/202554129
Revealing the ages of metal-rich RR Lyrae via kinematic label transfer
HanYuan Zhāng, Giuliano Iorio, Vasily Belokurov, N Wyn Evans, Alexey Bobrick and Valentina D’Orazi Monthly Notices of the Royal Astronomical Society 544(2) 2493 (2025) https://doi.org/10.1093/mnras/staf1789
The role of asteroseismology in understanding mass-loss in red giants
Advancing the accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
J. S. Thomsen, A. Miglio, K. Brogaard, J. Montalbán, M. Tailo, W. E. van Rossem, G. Casali, D. Jones, T. Arentoft, L. Casagrande, D. Sebastian, G. Buldgen, A. H. M. J. Triaud, M. Matteuzzi, A. Stokholm, M. N. Lund, B. Mosser, P. F. L. Maxted, J. Southworth, J. T. Gadeberg, N. Koivisto, Z. Gray, V. Pinter, K. Matilainen, A. A. Djupvik, et al. Astronomy & Astrophysics 699 A152 (2025) https://doi.org/10.1051/0004-6361/202453347
Evidence that Mass Loss on the Red Giant Branch Decreases with Metallicity