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20042026
most citedA new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase

1k citations · 3.8k across the 67 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.SR2019★ 144 cited

YBC, a stellar bolometric corrections database with variable extinction coefficients: an application to PARSEC isochrones

Yang Chen, Léo Girardi, Xiaoting Fu +7

We present the \texttt{YBC} database of stellar bolometric corrections (BCs), available at \url{http://stev.oapd.inaf.it/YBC}. We homogenize widely-used theoretical stellar spectra…

astro-ph.SR2019★ 33 cited

Evolutionary models for ultracool dwarfs

Catarina S. Fernandes, Valerie Van Grootel, Sebastien J. A. J. Salmon +5

Ultracool dwarfs have emerged as key targets for searches of transiting exoplanets. Precise estimates of the host parameters (including mass, age, and radius) are fundamental to co…

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★ 28 cited

A Dramatic Decrease in Carbon Star Formation in M31

M. L. Boyer, B. F. Williams, B. Aringer +8

We analyze resolved stellar near-infrared photometry of 21 HST fields in M31 to constrain the impact of metallicity on the formation of carbon stars. Observations of nearby galaxie…

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★ 57 cited

An extensive grid of DARWIN models for M-type AGB stars I. Mass-loss rates and other properties of dust-driven winds

S. Bladh, S. Liljegren, S. Höfner +2

The purpose of this work is to present an extensive grid of dynamical atmosphere and wind models for M-type AGB stars, covering a wide range of relevant stellar parameters. We used…