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Challenges in Forming Millisecond Pulsar–Black Holes from Isolated Binaries
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ExoMol line lists – LXII. Ro-vibrational energy levels and line strengths for the propadienediylidene (C3) in its ground electronic state
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The impact of third dredge-up on the mass loss of Mira variables
S. Uttenthaler, S. Shetye, A. Nanni, B. Aringer, K. Eriksson, I. McDonald, D. Gobrecht, S. Höfner, U. Wolter, S. Cristallo and K. Bernhard Astronomy & Astrophysics 690 A393 (2024) https://doi.org/10.1051/0004-6361/202451708
The formation and cosmic evolution of dust in the early Universe: I. Dust sources
Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud
K. Antoniadis, A. Z. Bonanos, S. de Wit, E. Zapartas, G. Munoz-Sanchez and G. Maravelias Astronomy & Astrophysics 686 A88 (2024) https://doi.org/10.1051/0004-6361/202449383
Dust formation in common envelope binary interaction – I: 3D simulations using the Bowen approximation
Miguel González-Bolívar, Orsola De Marco, Luis C Bermúdez-Bustamante, Lionel Siess and Daniel J Price Monthly Notices of the Royal Astronomical Society 527(3) 9145 (2023) https://doi.org/10.1093/mnras/stad3748
Global 3D radiation-hydrodynamical models of AGB stars with dust-driven winds
Relation of Observable Stellar Parameters to Mass-loss Rate of AGB Stars in the LMC
Henry A. Prager, Lee Anne Willson, Massimo Marengo and Michelle J. Creech-Eakman The Astrophysical Journal 941(1) 44 (2022) https://doi.org/10.3847/1538-4357/ac9e57
Light and colour variations of Mira variables in the Small Magellanic Cloud
Yoshifusa Ita, John W Menzies, Patricia A Whitelock, et al. Monthly Notices of the Royal Astronomical Society 500(1) 82 (2020) https://doi.org/10.1093/mnras/staa3251
Giants eating giants: mass loss and giant planets modifying the luminosity of the tip of the giant branch
magritte, a modern software library for 3D radiative transfer: I. Non-LTE atomic and molecular line modelling
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ATOMIUM: A high-resolution view on the highly asymmetric wind of the AGB starπ1Gruis
Constraining Stellar Parameters and Atmospheric Dynamics of the Carbon AGB star V Oph
Gioia Rau, Keiichi Ohnaka, Markus Wittkowski, Vladimir Airapetian and Kenneth G. Carpenter The Astrophysical Journal 882(1) 37 (2019) https://doi.org/10.3847/1538-4357/ab3419
An extensive grid of DARWIN models for M-type AGB stars
Developing a self-consistent AGB wind model – I. Chemical, thermal, and dynamical coupling
Jels Boulangier, N Clementel, A J van Marle, L Decin and A de Koter Monthly Notices of the Royal Astronomical Society 482(4) 5052 (2019) https://doi.org/10.1093/mnras/sty2560
HST/GHRS Observations of Cool, Low-gravity Stars. VI. Mass-loss Rates and Wind Parameters for M Giants
The curious case of II Lup: a complex morphology revealed with SAM/NACO and ALMA
Foteini Lykou, A A Zijlstra, J Kluska, et al. Monthly Notices of the Royal Astronomical Society 480(1) 1006 (2018) https://doi.org/10.1093/mnras/sty1903
High-resolution observations of gas and dust around Mira using ALMA and SPHERE/ZIMPOL
Constraining dust properties in circumstellar envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of carbon dust
Ambra Nanni, Paola Marigo, Martin A. T. Groenewegen, et al. Monthly Notices of the Royal Astronomical Society 462(2) 1215 (2016) https://doi.org/10.1093/mnras/stw1681
Connecting the evolution of thermally pulsing asymptotic giant branch stars to the chemistry in their circumstellar envelopes – I. Hydrogen cyanide
Paola Marigo, Emanuele Ripamonti, Ambra Nanni, Alessandro Bressan and Léo Girardi Monthly Notices of the Royal Astronomical Society 456(1) 23 (2016) https://doi.org/10.1093/mnras/stv2547
Near-infrared spectro-interferometry of Mira variables and comparisons to 1D dynamic model atmospheres and 3D convection simulations
Evolution of thermally pulsing asymptotic giant branch stars – II. Dust production at varying metallicity
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Polarimetric studies of carbon stars at high Galactic latitude
Vibration-rotation pattern in acetylene. II. Introduction of Coriolis coupling in the global model and analysis of emission spectra of hot acetylene around 3 μm
Badr Amyay, Séverine Robert, Michel Herman, André Fayt, Balakrishna Raghavendra, Audrey Moudens, Jonathan Thiévin, Bertrand Rowe and Robert Georges The Journal of Chemical Physics 131(11) (2009) https://doi.org/10.1063/1.3200928
Low temperature Rosseland opacities with varied abundances of carbon and nitrogen