Search Results - "Aringer, B."
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Synthetic photometry for M and K giants and stellar evolution: hydrostatic dust-free model atmospheres and chemical abundances
Published in Monthly notices of the Royal Astronomical Society (21-04-2016)“…Based on a grid of hydrostatic spherical comarcs models for cool stars, we have calculated observable properties of these objects, which will be mainly used in…”
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A Dramatic Decrease in Carbon Star Formation in M31
Published in The Astrophysical journal (10-07-2019)“…We analyze resolved stellar near-infrared photometry of 21 Hubble Space Telescope (HST) fields in M31 to constrain the impact of metallicity on the formation…”
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3
Carbon stars with increased oxygen and nitrogen abundances: hydrostatic dust-free model atmospheres
Published in Monthly notices of the Royal Astronomical Society (01-08-2019)“…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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Understanding AGB evolution in Galactic bulge stars from high-resolution infrared spectroscopy
Published in Monthly notices of the Royal Astronomical Society (01-08-2015)“…An analysis of high-resolution near-infrared spectra of a sample of 45 asymptotic giant branch (AGB) stars towards the Galactic bulge is presented. The sample…”
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5
Molecular Opacities for Low-Mass Metal-poor AGB Stars Undergoing the Third Dredge-up
Published in The Astrophysical journal (20-09-2007)“…The concomitant overabundances of C, N, and s-process elements are commonly ascribed to the complex interplay of nucleosynthesis, mixing, and mass loss taking…”
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IS THERE A METALLICITY CEILING TO FORM CARBON STARS?—A NOVEL TECHNIQUE REVEALS A SCARCITY OF C STARS IN THE INNER M31 DISK
Published in The Astrophysical journal (01-09-2013)“…We use medium-band near-infrared (NIR) Hubble Space Telescope WFC3 photometry with model NIR spectra of asymptotic giant branch (AGB) stars to develop a new…”
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Temporal Changes in the Infrared Spectra of Magellanic Carbon Stars
Published in Galaxies (01-10-2024)“…The Medium-Resolution Spectrometer on the Mid-Infrared Instrument on the JWST obtained spectra of three carbon stars in the Large Magellanic Cloud. Two of the…”
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A CH star in the globular cluster NGC 6426
Published in Monthly notices of the Royal Astronomical Society. Letters (01-10-2012)“…ABSTRACT We report on the serendipitous discovery of a carbon star near the centre of the low‐metallicity globular cluster NGC 6426. We determined its…”
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The Fluorine Abundance in a Galactic Bulge AGB Star Measured from CRIRES Spectra
Published in The Astrophysical journal (20-07-2008)“…We present measurements of the fluorine abundance in a Galactic bulge asymptotic giant branch (AGB) star. The measurements were performed using high-resolution…”
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10
Elemental abundances in AGB stars and the formation of the Galactic bulge
Published in EPJ Web of conferences (01-01-2012)“…We obtained high-resolution near-IR spectra of 45 AGB stars located in the Galactic bulge. The aim of the project is to determine key elemental abundances in…”
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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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12
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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Silicate dust emission in sr variables
Published in Astrophysics and space science (01-02-1995)Get full text
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14
CO observations of semiregular variables
Published in Astrophysics and space science (01-02-1995)Get full text
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Sio observations of mass-losing AGB stars
Published in Astrophysics and space science (01-02-1995)Get full text
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16
AESOPUS 2.0: Low-Temperature Opacities with Solid Grains
Published 23-10-2023“…In this study we compute the equation of state and Rosseland mean opacity from temperatures of T~30000 K down to T~400 K, pushing the capabilities of the…”
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17
The impact of third dredge-up on the mass loss of Mira variables
Published 29-09-2024“…Context: The details of the mass-loss process in the late stages of low- and intermediate-mass stellar evolution are not well understood, in particular its…”
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An extensive grid of DARWIN models for M-type AGB stars I. Mass-loss rates and other properties of dust-driven winds
Published 17-05-2019“…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…”
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Carbon star wind models at solar and sub-solar metallicities: a comparative study. I. Mass loss and the properties of dust-driven winds
Published 14-02-2019“…A&A 623, A119 (2019) The atmospheres and winds of C-type AGB stars are modeled with the 1D spherically symmetric radiation-hydrodynamical code DARWIN. To…”
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20
An impressionist view of V Hydrae. When MATISSE paints Asymmetric Giant Blobs
Published 13-05-2024“…A&A 687, A306 (2024) Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this work,…”
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