Search Results - "Bressan, Alessandro"
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The mass spectrum of compact remnants from the parsec stellar evolution tracks
Published in Monthly notices of the Royal Astronomical Society (21-08-2015)“…The mass spectrum of stellar mass black holes (BHs) is highly uncertain. Dynamical mass measurements are available only for few (∼10) BHs in X-ray binaries,…”
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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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Formation of black holes in the pair-instability mass gap: Evolution of a post-collision star
Published in Monthly notices of the Royal Astronomical Society (01-09-2022)“…ABSTRACT The detection of GW190521 by the LIGO–Virgo collaboration has revealed the existence of black holes (BHs) in the pair-instability (PI) mass gap. Here,…”
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Formation of GW190521 from stellar evolution: the impact of the hydrogen-rich envelope, dredge-up, and 12C(α, γ)16O rate on the pair-instability black hole mass gap
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT Pair-instability (PI) is expected to open a gap in the mass spectrum of black holes (BHs) between ≈40–65 and ≈120 M⊙. The existence of the mass gap is…”
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Binary black holes in the pair instability mass gap
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT Pair instability (PI) and pulsational PI prevent the formation of black holes (BHs) with mass ≳60 M⊙ from single star evolution. Here, we investigate…”
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Lithium evolution in metal-poor stars: from pre-main sequence to the Spite plateau
Published in Monthly notices of the Royal Astronomical Society (21-09-2015)“…Lithium abundance derived in metal-poor main-sequence (MS) stars is about three times lower than the value of primordial Li predicted by the standard big bang…”
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Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
Published in The Astrophysical journal (10-01-2020)“…We investigate the impact of stellar rotation on the formation of black holes (BHs) by means of our population synthesis code sevn. Rotation affects the mass…”
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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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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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The host galaxies of double compact objects merging in the local Universe
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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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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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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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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The Role of the Third Dredge-up and Mass Loss in Shaping the Initial–Final Mass Relation of White Dwarfs
Published in The Astrophysical journal (01-03-2024)“…Abstract The initial–final mass relation (IFMR) plays a crucial role in understanding stellar structure and evolution by linking a star’s initial mass to the…”
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Uncertainties on near-core mixing in red-clump stars: effects on the period spacing and on the luminosity of the AGB bump
Published in Monthly notices of the Royal Astronomical Society (01-11-2015)“…Low-mass stars in the He-core-burning (HeCB) phase play a major role in stellar, galactic, and extragalactic astrophysics. The ability to predict accurately…”
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ÆSOPUS 2.1: Low-temperature Opacities Extended to High Pressure
Published in The Astrophysical journal (01-11-2024)“…Abstract We address the critical need for accurate Rosseland mean gas opacities in high-pressure environments, spanning temperatures from 100 K to 32,000 K…”
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A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors
Published in The Astrophysical journal (01-01-2024)“…Abstract We calculate new evolutionary models of rotating primordial very massive stars, with initial mass from 100 M ⊙ to 200 M ⊙ , for two values of the…”
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