Search Results - "Aringer, Bernhard"
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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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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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Carbon star formation as seen through the non-monotonic initial–final mass relation
Published in Nature astronomy (01-11-2020)“…The initial–final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR…”
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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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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…Abstract The thermally pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our…”
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Estimating the dust production rate of carbon stars in the Small Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)Get full text
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The mass-loss, expansion velocities, and dust production rates of carbon stars in the Magellanic Clouds
Published in Monthly notices of the Royal Astronomical Society (21-07-2019)“…ABSTRACT The properties of carbon stars in the Magellanic Clouds (MCs) and their total dust production rates are predicted by fitting their spectral energy…”
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EVOLUTION OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS. IV. CONSTRAINING MASS LOSS AND LIFETIMES OF LOW MASS, LOW METALLICITY AGB STARS
Published in The Astrophysical journal (20-07-2014)“…The evolution and lifetimes of thermally pulsating asymptotic giant branch (TP-AGB) stars suffer from significant uncertainties. In this work, we analyze the…”
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Evolutionary Models for Ultracool Dwarfs
Published in The Astrophysical journal (10-07-2019)“…Ultracool dwarfs (UCDs) have emerged as key targets for searches of transiting exoplanets. Precise estimates of the host parameters (including mass, age, and…”
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THE PTI CARBON STAR ANGULAR SIZE SURVEY: EFFECTIVE TEMPERATURES AND NON-SPHERICITY
Published in The Astrophysical journal (20-09-2013)“…We report new interferometric angular diameter observations of 41 carbon stars observed with the Palomar Testbed Interferometer. Two of these stars are CH…”
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Constraining dust properties in circumstellar envelopes of C-stars in the Small Magellanic Cloud: optical constants and grain size of carbon dust
Published in Monthly notices of the Royal Astronomical Society (21-10-2016)“…We present a new approach aimed at constraining the typical size and optical properties of carbon dust grains in circumstellar envelopes (CSEs) of carbon-rich…”
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Synthetic photometry for carbon-rich giants. V. Effects of grain-size-dependent dust opacities
Published 17-03-2023“…A&A 673, A21 (2023) The properties and the evolution of asymptotic giant branch (AGB) stars are strongly influenced by their mass loss through a stellar wind…”
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Low-Temperature Gas Opacities with AESOPUS 2.0
Published 16-10-2022“…This work introduces new low-temperature gas opacities, in the range 3.2 <= log(T/K) <= 4.5, computed with the AESOPUS code under the assumption of…”
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Dynamic atmospheres and winds of cool luminous giants, II. Gradual Fe enrichment of wind-driving silicate grains
Published 29-10-2021“…A&A 657, A109 (2022) The winds observed around AGB stars are generally attributed to radiation pressure on dust formed in the dynamical atmospheres of these…”
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A multi-method approach to the outer layers of AGB stars
Published in Astronomische Nachrichten (2007)Get full text
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Carbon stars with increased oxygen and nitrogen abundances: hydrostatic dust-free model atmospheres
Published 22-05-2019“…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]…”
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How important are metal-poor AGB stars as cosmic dust producers?
Published 18-05-2015“…The efficiency of dust formation in oxygen-rich AGB stars should (in theory) be metallicity dependent since they are not producing their own raw material for…”
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Dynamic atmospheres and winds of cool luminous giants, I. Al$_2$O$_3$ and silicate dust in the close vicinity of M-type AGB stars
Published 31-05-2016“…A&A 594, A108 (2016) High spatial resolution techniques have given valuable insights into the mass loss mechanism of AGB stars, which presumably involves a…”
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