Search Results - "Hoefner, S"

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    On the Evolution of Comets by Guilbert-Lepoutre, A., Besse, S., Mousis, O., Ali-Dib, M., Höfner, S., Koschny, D., Hager, P.

    Published in Space science reviews (01-12-2015)
    “…Studying comets is believed to bring invaluable clues on the formation and evolution of our planetary system. In comparison to planets, they have undergone…”
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    On the Evolution of Comets Review article by A., Guilbert-Lepoutre, Besse, S., Mousis, O., Ali-Dib, M., Hoefner, S., Koschny, D., Hager, P.

    Published in Space science reviews (2015)
    “…Studying comets is believed to bring invaluable clues on the formation and evolution of our planetary system. In comparison to planets, they have undergone…”
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    Journal Article
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    Dust Formation and Winds around Evolved Stars: The Good, the Bad and the Ugly Cases by Hoefner, S

    Published 30-03-2009
    “…Cool luminous giants, in particular asymptotic giant branch stars, are among the most important sources of cosmic dust. Their extended dynamical atmospheres…”
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    Headwind: Modelling Mass Loss of AGB Stars, Against All Odds by Hoefner, S

    Published 16-02-2007
    “…The intricate interplay of atmospheric shock waves and a complex, variable radiation field with non-equilibrium dust formation presents a considerable…”
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    Synthetic radii and visibilities for pulsating red giants by Hron, Josef, Nowotny, Walter, Gautschy-Loidl, Rita, Hoefner, Susanne

    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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    VLTI-GRAVITY measurements of cool evolved stars: I. Variable photosphere and extended atmosphere of the Mira star R Peg by Wittkowski, M, Rau, G, Chiavassa, A, Hoefner, S, Scholz, M, Wood, P. R, de Wit, W. J, Eisenhauer, F, Haubois, X, Paumard, T

    Published 14-05-2018
    “…A&A 613, L7 (2018) Dynamic model atmospheres of Mira stars predict variabilities in the photospheric radius and in atmospheric molecular layers which are not…”
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    Near-infrared spectro-interferometry of Mira variables and comparisons to 1D dynamic model atmospheres and 3D convection simulations by Wittkowski, M, Chiavassa, A, Freytag, B, Scholz, M, Hoefner, S, Karovicova, I, Whitelock, P. A

    Published 11-01-2016
    “…A&A 587, A12 (2016) We obtained a total of 20 near-infrared K-band spectro-interferometric snapshot observations of the Mira variables o Cet, R Leo, R Aqr, X…”
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    Synthetic photometry for carbon-rich giants. III. Tracing the sequence of mass-losing galactic C-type Miras by Nowotny, W, Aringer, B, Hoefner, S, Eriksson, K

    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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    Line formation in AGB atmospheres including velocity effects. Molecular line profile variations of long period variables by Nowotny, W, Hoefner, S, Aringer, B

    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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    Winds of M- and S-type AGB stars: an unorthodox suggestion for the driving mechanism by Hoefner, S, Andersen, A. C

    Published 16-02-2007
    “…Astron.Astrophys.465:L39,2007 Current knowledge suggests that the dust-driven wind scenario provides a realistic framework for understanding mass loss from…”
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    Three-component modeling of C-rich AGB star winds III. Micro-physics of drift-dependent dust formation by Sandin, C, Hoefner, S

    Published 30-09-2003
    “…Astron.Astrophys. 413 (2004) 789 A proper treatment of the non-equilibrium dust formation process is crucial in models of AGB star winds. In this paper the…”
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    Three-component modeling of C-rich AGB star winds. II. The effects of drift in long-period variables by Sandin, C, Hoefner, S

    Published 15-04-2003
    “…Astron.Astrophys. 404 (2003) 789 We present three-component wind models for carbon rich pulsating AGB stars. In particular we study the effects of drift in…”
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    Three-component modeling of C-rich AGB star winds I. Method and first results by Sandin, C, Hoefner, S

    Published 13-11-2002
    “…Astron.Astrophys. 398 (2003) 253-266 Radiative acceleration of newly-formed dust grains and transfer of momentum from the dust to the gas plays an important…”
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