Search Results - "Girardi, Léo"
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Red Clump Stars
Published in Annual review of astronomy and astrophysics (19-09-2016)“…Low-mass stars in their core-helium-burning stage define the sharpest feature present in the color-magnitude diagrams of nearby galaxy systems: the red clump…”
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parsec evolutionary tracks of massive stars up to 350 M⊙ at metallicities 0.0001 ≤ Z ≤ 0.04
Published in Monthly notices of the Royal Astronomical Society (01-09-2015)“…We complement the parsec data base of stellar evolutionary tracks with new models of massive stars, from the pre-main-sequence phase to the central carbon…”
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Improving PARSEC models for very low mass stars
Published in Monthly notices of the Royal Astronomical Society (01-11-2014)“…Many stellar models present difficulties in reproducing basic observational relations of very low mass stars (VLMS), including the mass-radius relation and the…”
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Updated Low-temperature Gas Opacities with ÆSOPUS 2.0
Published in The Astrophysical journal (01-12-2022)“…Abstract This work introduces new low-temperature gas opacities in the range 3.2 ≲ log ( T / K ) ≲ 4.5 computed with the Æ SOPUS code under the assumption of…”
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Extended Main-sequence Turn-offs in Intermediate-age Star Clusters: Stellar Rotation Diminishes, but Does Not Eliminate, Age Spreads
Published in The Astrophysical journal (01-09-2017)“…Extended main-sequence turn-off (eMSTO) regions are a common feature in color-magnitude diagrams of young- and intermediate-age star clusters in the Magellanic…”
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Evolution of thermally pulsing asymptotic giant branch stars - I. The colibri code
Published in Monthly notices of the Royal Astronomical Society (01-09-2013)“…We present the colibri code for computing the evolution of stars along the thermally pulsing asymptotic giant branch (TP-AGB) phase. Compared to purely…”
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New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies
Published in Monthly notices of the Royal Astronomical Society (21-12-2014)“…We extend the PARSEC library of stellar evolutionary tracks by computing new models of massive stars, from 14 to 350 M⊙. The input physics is the same used in…”
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PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
Published in Monthly notices of the Royal Astronomical Society (21-11-2012)“…Abstract We present the updated version of the code used to compute stellar evolutionary tracks in Padova. It is the result of a thorough revision of the major…”
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Evolution of thermally pulsing asymptotic giant branch stars - II. Dust production at varying metallicity
Published in Monthly notices of the Royal Astronomical Society (21-09-2013)“…We present the dust ejecta of the new stellar models for the thermally pulsing asymptotic giant branch (TP-AGB) phase computed with the colibri code. We use a…”
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Determining stellar parameters of asteroseismic targets: going beyond the use of scaling relations
Published in Monthly notices of the Royal Astronomical Society (17-01-2017)“…Abstract Asteroseismic parameters allow us to measure the basic stellar properties of field giants observed far across the Galaxy. Most of such determinations…”
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A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE
Published in The Astrophysical journal (20-01-2017)“…We introduce a new generation of PARSEC-COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB)…”
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A Study of Primordial Very Massive Star Evolution
Published in The Astrophysical journal (01-02-2023)“…Abstract We present new evolutionary models of primordial very massive stars with initial masses ranging from 100 to 1000 M ⊙ that extend from the main…”
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Evolution of thermally pulsing asymptotic giant branch stars - III. Dust production at supersolar metallicities
Published in Monthly notices of the Royal Astronomical Society (01-03-2014)“…We extend the formalism presented in our recent calculations of dust ejecta from the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase to the case of…”
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A New Interpretation of the Period-Luminosity Sequences of Long-period Variables
Published in The Astrophysical journal (01-10-2017)“…Period-luminosity (PL) sequences of long-period variables (LPVs) are commonly interpreted as different pulsation modes, but there is disagreement on the modal…”
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CHEMICAL CARTOGRAPHY WITH APOGEE: METALLICITY DISTRIBUTION FUNCTIONS AND THE CHEMICAL STRUCTURE OF THE MILKY WAY DISK
Published in The Astrophysical journal (01-08-2015)“…ABSTRACT Using a sample of 69,919 red giants from the SDSS-III/APOGEE Data Release 12, we measure the distribution of stars in the [ /Fe] versus [Fe/H] plane…”
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EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. V. CONSTRAINING THE MASS LOSS AND LIFETIMES OF INTERMEDIATE-MASS, LOW-METALLICITY AGB STARS
Published in The Astrophysical journal (10-05-2016)“…ABSTRACT Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few Myr), yet their cool effective temperatures, high…”
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Modelling long-period variables – I. A new grid of O-rich and C-rich pulsation models
Published in Monthly notices of the Royal Astronomical Society (01-01-2019)Get full text
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Modelling long-period variables – II. Fundamental mode pulsation in the non-linear regime
Published in Monthly notices of the Royal Astronomical Society (01-01-2021)“…ABSTRACT Long-period variability in luminous red giants has several promising applications, all of which require models able to accurately predict pulsation…”
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ÆSOPUS 2.0: Low-temperature Opacities with Solid Grains
Published in The Astrophysical journal (01-01-2024)“…Abstract In this study we compute the equation of state and Rosseland mean opacity from temperatures of T ≃ 30,000 K down to T ≃ 400 K, pushing the…”
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