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Understanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST
E. Marini, F. Dell'Agli, M. A. T. Groenewegen +6
Carbon stars have been and are extensively studied, given their complex internal structure and their peculiar chemical composition, which make them living laboratories to test stel…
Are extreme AGB stars post-common envelope binaries?
F. Dell'Agli, E. Marini, F. D'Antona +6
Modelling dust formation in single stars evolving through the carbon-star stage of the asymptotic giant branch (AGB) reproduces well the mid-infrared colours and magnitudes of most…
Extended view on the dust shells around two carbon stars
M. Mečina, B. Aringer, W. Nowotny +4
Stars on the asymptotic giant branch (AGB) lose considerable amounts of matter through their dust-driven stellar winds. A number of such sources have been imaged by Herschel/PACS,…
Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud
Giada Pastorelli, Paola Marigo, Léo Girardi +18
Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our interpretation of the spectral energy…
The flux-weighted gravity-luminosity relation of Galactic classical Cepheids
M. A. T. Groenewegen
The flux-weighted gravity-luminosity relation (FWGLR) is investigated for a sample of 477 classical Cepheids (CCs), including stars that have been classified in the literature as s…
Analysing the spectral energy distributions of Galactic classical Cepheids
M. A. T. Groenewegen
(abridged) Spectral energy distributions (SEDs) were constructed for a sample of 477 classical cepheids (CCs). The SEDs were fitted with a dust radiative transfer code. Four stars…