Search Results - "Danilovich, T."
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Chemical modelling of dust–gas chemistry within AGB outflows – II. Effect of the dust-grain size distribution
Published in Monthly notices of the Royal Astronomical Society (01-06-2020)“…ABSTRACT Asymptotic giant branch (AGB) stars are, together with supernovae, the main contributors of stellar dust to the interstellar medium (ISM). Dust grains…”
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(Sub)stellar companions shape the winds of evolved stars
Published in Science (American Association for the Advancement of Science) (18-09-2020)“…Complex stellar winds from evolved stars Stars less than eight times the mass of the Sun end their lives as planetary nebulae, structures of ionized gas thrown…”
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3
Sensitivity study of chemistry in AGB outflows using chemical kinetics
Published in Monthly notices of the Royal Astronomical Society (02-05-2023)“…ABSTRACT Asymptotic giant branch (AGB) stars shed a significant amount of their mass in the form of a stellar wind, creating a vast circumstellar envelope…”
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Modelling predicts a molecule-rich disc around the AGB star L2 Puppis
Published in Monthly notices of the Royal Astronomical Society (01-07-2024)“…ABSTRACT The nearby oxygen-rich AGB star L$_2$ Pup hosts a well-studied nearly edge-on disc. To date, discs around AGB stars have not been chemically studied…”
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5
An ALMA view of CS and SiS around oxygen-rich AGB stars
Published in Monthly notices of the Royal Astronomical Society (21-03-2019)Get full text
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An ALMA view of SO and SO2 around oxygen-rich AGB stars
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT We present and analyse SO and SO2, recently observed with high angular resolution and sensitivity in a spectral line survey with ALMA, for two…”
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Rotational Spectra of Vibrationally Excited AlO and TiO in Oxygen-rich Stars
Published in The Astrophysical journal (01-12-2020)“…Rotational transitions in vibrationally excited AlO and TiO-two possible precursors of dust-were observed in the 300 GHz range (1 mm wavelength) toward the…”
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Constraints on Metal Oxide and Metal Hydroxide Abundances in the Winds of AGB Stars: Potential Detection of FeO in R Dor
Published in The Astrophysical journal (10-03-2018)“…Using the Atacama Large Millimeter/submillimeter Array (ALMA), we observed the stellar wind of two oxygen-rich asymptotic giant branch stars, IK Tau and R Dor,…”
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Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
Published in Nature astronomy (01-05-2019)“…In 1981, the idea of a superwind that ends the life of cool giant stars was proposed 1 . Extreme oxygen-rich giants, OH/IR stars, develop superwinds with the…”
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The fundamental manifold of spiral galaxies: ordered versus random motions and the morphology dependence of the Tully-Fisher relation
Published in Monthly notices of the Royal Astronomical Society (2014)“…We investigate the morphology dependence of the Tully-Fisher (TF) relation, and the expansion of the relation into a three-dimensional manifold defined by…”
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Chemical tracers of a highly eccentric AGB–main-sequence star binary
Published in Nature astronomy (2024)“…Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB)…”
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Author Correction: Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
Published in Nature astronomy (01-05-2019)“…In the version of this Letter originally published, the caption of Fig. 2 incorrectly said J = 3–2; it should have said J = 2–1. This has now been corrected…”
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The salty emission of the intermediate-mass AGB star OH 30.1−0.7
Published in Monthly notices of the Royal Astronomical Society (18-11-2024)“…Abstract We analyse continuum and molecular emission, observed with ALMA, from the dust-enshrouded intermediate-mass AGB star OH 30.1 −0.7. We find a secondary…”
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The unusual 3D distribution of NaCl around the AGB star IK Tau
Published 24-08-2023“…A&A 678, A85 (2023) NaCl is a diatomic molecule with a large dipole moment, which allows for its detection even at relatively small abundances. It has been…”
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Modelling predicts a molecule-rich disk around the AGB star L2 Puppis
Published 18-06-2024“…The nearby oxygen-rich AGB star L2 Pup hosts a well-studied nearly edge-on disk. To date, disks around AGB stars have not been chemically studied in detail. By…”
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16
Sensitivity study of chemistry in AGB outflows using chemical kinetics
Published 19-04-2023“…Asymptotic Giant Branch (AGB) stars shed a significant amount of their mass in the form of a stellar wind, creating a vast circumstellar envelope (CSE). Owing…”
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17
Chemical modelling of dust-gas chemistry within AGB outflows -- II. Effect of the dust-grain size distribution
Published 04-05-2020“…AGB stars are, together with supernovae, the main contributors of stellar dust to the interstellar medium (ISM). Dust grains formed by AGB stars are thought to…”
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The salty emission of the intermediate-mass AGB star OH 30.1 -0.7
Published 12-11-2024“…We analyse continuum and molecular emission, observed with ALMA, from the dust-enshrouded intermediate-mass AGB star OH 30.1 -0.7. We find a secondary peak in…”
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How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions -- The case of EP Aqr
Published 26-08-2020“…A&A 642, A142 (2020) High-angular-resolution observations of asymptotic giant branch (AGB) stars often reveal non-spherical morphologies for the gas and dust…”
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An ALMA view of SO and SO$_2$ around oxygen-rich AGB stars
Published 09-03-2020“…We present and analyse SO and SO$_2$, recently observed with high angular resolution and sensitivity in a spectral line survey with ALMA, for two oxygen-rich…”
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