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The age of 47 Tuc from self-consistent isochrone fits to colour–magnitude diagrams and the eclipsing member V69
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The more the merrier: grid based modelling of Kepler dwarfs with 5-dimensional stellar grids
Standing on the Shoulders of Dwarfs: the Kepler Asteroseismic LEGACY Sample. II. Radii, Masses, and Ages
Víctor Silva Aguirre, Mikkel N. Lund, H. M. Antia, Warrick H. Ball, Sarbani Basu, Jørgen Christensen-Dalsgaard, Yveline Lebreton, Daniel R. Reese, Kuldeep Verma, Luca Casagrande, Anders B. Justesen, Jakob R. Mosumgaard, William J. Chaplin, Timothy R. Bedding, Guy R. Davies, Rasmus Handberg, Günter Houdek, Daniel Huber, Hans Kjeldsen, David W. Latham, Timothy R. White, Hugo R. Coelho, Andrea Miglio and Ben Rendle The Astrophysical Journal 835(2) 173 (2017) https://doi.org/10.3847/1538-4357/835/2/173
Red supergiants as supernova progenitors
Ben Davies Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 375(2105) 20160270 (2017) https://doi.org/10.1098/rsta.2016.0270
A comparative study of multiwavelength theoretical and observed light curves of Cepheid variables
Anupam Bhardwaj, Shashi M. Kanbur, Marcella Marconi, et al. Monthly Notices of the Royal Astronomical Society 466(3) 2805 (2017) https://doi.org/10.1093/mnras/stw3256
Interpretation of the BRITE oscillation data of the hybrid pulsator ν Eridani: a call for the modification of stellar opacities
J. Daszyńska-Daszkiewicz, A. A. Pamyatnykh, P. Walczak, et al. Monthly Notices of the Royal Astronomical Society 466(2) 2284 (2017) https://doi.org/10.1093/mnras/stw3315
Red supergiant stars in NGC 4449, NGC 5055 (M63) and NGC 5457 (M101)
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On the relevance of bubbles and potential flows for stellar convection
M. M. Miller Bertolami, M. Viallet, V. Prat, W. Barsukow and A. Weiss Monthly Notices of the Royal Astronomical Society 457(4) 4441 (2016) https://doi.org/10.1093/mnras/stw203
On the red giant branch mass loss in 47 Tucanae: Constraints from the horizontal branch morphology
Theory of stellar convection – II. First stellar models
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CONSTRAINTS ON THE DISTANCE MODULI, HELIUM AND METAL ABUNDANCES, AND AGES OF GLOBULAR CLUSTERS FROM THEIR RR LYRAE AND NON-VARIABLE HORIZONTAL-BRANCH STARS. I. M3, M15, AND M92
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Jieun Choi, Aaron Dotter, Charlie Conroy, Matteo Cantiello, Bill Paxton and Benjamin D. Johnson The Astrophysical Journal 823(2) 102 (2016) https://doi.org/10.3847/0004-637X/823/2/102
SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
Non-LTE line formation of Fe in late-type stars – III. 3D non-LTE analysis of metal-poor stars
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Calibrating convective-core overshooting with eclipsing binary systems
Young α-enriched giant stars in the solar neighbourhood
Marie Martig, Hans-Walter Rix, Victor Silva Aguirre, et al. Monthly Notices of the Royal Astronomical Society 451(2) 2230 (2015) https://doi.org/10.1093/mnras/stv1071
DIVISION G COMMISSION 36: THEORY OF STELLAR ATMOSPHERES
Ages and fundamental properties ofKeplerexoplanet host stars from asteroseismology
V. Silva Aguirre, G. R. Davies, S. Basu, et al. Monthly Notices of the Royal Astronomical Society 452(2) 2127 (2015) https://doi.org/10.1093/mnras/stv1388
Diagnostics of stellar modelling from spectroscopy and photometry of globular clusters
George C. Angelou, Valentina D'Orazi, Thomas N. Constantino, et al. Monthly Notices of the Royal Astronomical Society 450(3) 2423 (2015) https://doi.org/10.1093/mnras/stv770
Stellar models with mixing length andT(τ) relations calibrated on 3D convection simulations