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20162026
most citedConstraining the thermally-pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud

217 citations · 904 across the 20 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR2020

On the mass and metallicity distribution of parent AGB stars of presolar SiC

Sergio Cristallo, Ambra Nanni, Gabriele Cescutti +5

The vast majority (>=90%) of presolar SiC grains identified in primitive meteorites are relics of ancient asymptotic giant branch (AGB) stars, whose ejecta were incorporated into t…

astro-ph.SR2020★ 175 cited

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…

astro-ph.SR2019★ 48 cited

The mass-loss, expansion velocities and dust production rates of carbon stars in the Magellanic Clouds

Ambra Nanni, Martin A. T. Groenewegen, Bernhard Aringer +5

The properties of carbon stars in the Magellanic Clouds (MCs) and their total dust production rates are predicted by fitting their spectral energy distributions (SED) over pre-comp…

astro-ph.SR2019★ 17 cited

Carbon stars with increased oxygen and nitrogen abundances: hydrostatic dust-free model atmospheres

Bernhard Aringer, Paola Marigo, Walter Nowotny +3

We have computed a grid of hydrostatic spherical COMARCS models for C stars covering metallicities from [Z/H]=0 to -2 and values of the carbon excess [C-O] from 6.41 to 9.15, plus…

astro-ph.SR2019★ 217 cited

Constraining the thermally-pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud

Giada Pastorelli, Paola Marigo, Léo Girardi +17

The thermally-pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar evolution and the models need…

astro-ph.SR2018

Optical properties of amorphous carbon dust around C-stars: new constraints from 2MASS and Gaia observations

Ambra Nanni

In this work the optical properties of amorphous carbon (amC) dust condensed around carbon(C)-stars are constrained by comparing the observations for the Large Magellanic Cloud C-s…