Search Results - "Nowotny, W"
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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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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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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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STEREO observations of long period variables
Published in Monthly notices of the Royal Astronomical Society (21-10-2012)“…Abstract Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecrafts have been analysed to search for very long period large amplitude…”
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STEREO observations of long period variables: STEREO observations of LPVs
Published in Monthly notices of the Royal Astronomical Society (21-10-2012)Get full text
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Pulsation-induced atmospheric dynamics in M-type AGB stars. Effects on wind properties, photometric variations and near-IR CO line profiles
Published 26-06-2017“…A&A 606, A6 (2017) Wind-driving in asymptotic giant branch (AGB) stars is commonly attributed to a two-step process. First, matter in the stellar atmosphere is…”
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Extended view on the dust shells around two carbon stars
Published 28-10-2020“…A&A 644, A66 (2020) Stars on the asymptotic giant branch (AGB) lose considerable amounts of matter through their dust-driven stellar winds. A number of such…”
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Dust-driven winds of AGB stars: The critical interplay of atmospheric shocks and luminosity variations
Published 22-03-2016“…A&A 589, A130 (2016) Winds of AGB stars are thought to be driven by a combination of pulsation-induced shock waves and radiation pressure on dust. In dynamic…”
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(Re)Solving the dynamic atmospheres of carbon-rich giants
Published in Astronomische Nachrichten (2005)Get full text
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Synthetic radii and visibilities for pulsating red giants
Published in Astrophysics and space science (01-08-2003)“…We present synthetic radii and visibilities in the IR, based on hydrostatic and dynamic model atmospheres of carbon stars. The differences between these two…”
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Synthetic photometry for carbon-rich giants. III. Tracing the sequence of mass-losing galactic C-type Miras
Published 15-02-2013“…With the help of model calculations we aim at reproducing the observational photometric findings for a large sample of well-characterised galactic C-type Mira…”
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Modelling the atmosphere of the carbon-rich Mira RU Vir
Published 31-08-2015“…A&A 583, A106 (2015) Context. We study the atmosphere of the carbon-rich Mira RU Vir using the mid-infrared high spatial resolution interferometric…”
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13
Line formation in AGB atmospheres including velocity effects. Molecular line profile variations of long period variables
Published 09-02-2010“…The atmospheres of evolved red giants are considerably influenced by pulsations of the stellar interiors and developing stellar winds. The resulting complex…”
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Carbon stars in the X-Shooter Spectral Library: II. Comparison with models
Published 02-02-2017“…A&A 601, A141 (2017) In a previous paper, we assembled a collection of medium-resolution spectra of 35 carbon stars, covering optical and near-infrared…”
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Aperture synthesis imaging of the carbon AGB star R Sculptoris: Detection of a complex structure and a dominating spot on the stellar disk
Published 08-02-2017“…A&A 601, A3 (2017) We present near-infrared interferometry of the carbon-rich asymptotic giant branch (AGB) star R Sculptoris. The visibility data indicate a…”
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Detection of an asymmetry in the envelope of the carbon Mira R Fornacis using VLTI/MIDI
Published 19-07-2012“…Aims. We present a study of the envelope morphology of the carbon Mira R For with VLTI/MIDI. This object is one of the few asymptotic giant branch (AGB) stars…”
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Carbon stars in the X-shooter Spectral Library
Published 02-02-2016“…A&A 589, A36 (2016) We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-shooter instrument as part of the X-shooter Spectral…”
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Long-period variables in NGC147 and NGC185
Published 26-06-2011“…Previous studies on the stellar content of the two nearby dwarf galaxies NGC147 and NGC185 reveal a rich population of late-type giants in both systems,…”
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STEREO observations of long period variables
Published 07-06-2012“…Observations from the Heliospheric Imagers (HI-1) on both the STEREO spacecraft have been analysed to search for very long period large amplitude stellar…”
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Synthetic photometry for carbon rich giants, I. Hydrostatic dust-free models
Published 27-05-2009“…We study the spectroscopic and photometric properties of carbon stars. In the first paper of this series we focus on objects that can be described by…”
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