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  • Publications
    Sufficiency of near-surface water ice as a driver of dust activity on comets. Rethinking the old enigma

    Skorov, Y. V., Mokhtari, O., Macher, W., Reshetnyk, V., Markkanen, J., Zhao, Y., Thomas, N., Küppers, M., & Hartogh, P. (2024). Sufficiency of near-surface water ice as a driver of dust activity on comets. Rethinking the old enigma. Astronomy and Astrophysics, 689, A131. https://doi.org/10.1051/0004-6361/202449433

  • Publications
    Influence of the evolving stellar X-ray luminosity distribution on exoplanetary mass loss

    Penz, T., Micela, G., & Lammer, H. (2008). Influence of the evolving stellar X-ray luminosity distribution on exoplanetary mass loss. Astronomy and Astrophysics, 477, 309-314, doi:10.1051/0004-6361:20078364.

  • Publications
    The size distribution of magnetic bright points derived from Hinode/SOT observations

    Utz, D., Hanslmeier, A., Möstl, C., Muller, R., Veronig, A., & Muthsam, H. (2009). The size distribution of magnetic bright points derived from Hinode/SOT observations. Astronomy and Astrophysics, 498, 289–293, doi:10.1051/0004-6361/200810867.

  • Publications
    Noise properties of the CoRoT data: A planet-finding perspective

    Aigrain, S., Pont, F., Fressin, F., Alapini, A., Alonso, R., Auvergne, M., Barbieri, M., Barge, P., Bordé, P., Bouchy, F., Deeg, H., Reza, R., Deleuil, M., Dvorak, R., Erikson, A., Fridlund, M., Gondoin, P., Guterman, P., Jorda, L., ... Zucker, S. (2009). Noise properties of the CoRoT data: A planet-finding perspective. Astronomy and Astrophysics, 506, 425-429, doi:10.1051/0004-6361/200911885.

  • Publications
    The Schumann resonance: A tool for exploring the atmospheric environment and the subsurface of the planets and their satellites

    Simoes, F., Grard, R., Hamelin, M., López-Moreno, J. J., Schwingenschuh, K., Béghin, C., Berthelier, J.-J., Lebreton, J.-P., Molina-Cuberos, G. J., & Tokano, T. (2008). The Schumann resonance: A tool for exploring the atmospheric environment and the subsurface of the planets and their satellites. Science, 35, L03105, doi:10.1029/2007GL032594.

  • Publications
    Energetic neutral atoms as the explanation for the high-velocity hydrogen around HD 209458b

    Holmström, M., Ekenbäck, A., Selsis, F., Penz, T., Lammer, H., & Wurz, P. (2008). Energetic neutral atoms as the explanation for the high-velocity hydrogen around HD 209458b. Nature, 451, 970-972, doi:10.1038/nature06600.

  • Publications
    The Kepler-11 system: Evolution of the stellar high-energy emission and initial planetary atmospheric mass fractions

    Kubyshkina, D., Fossati, L., Mustill, A. J., Cubillos, P. E., Davies, M. B., Erkaev, N. V., Johnstone, C. P., Kislyakova, K. G., Lammer, H., Lendl, M., & Odert, P. (2019). The Kepler-11 system: Evolution of the stellar high-energy emission and initial planetary atmospheric mass fractions. Astronomy and Astrophysics, 632, A65. https://doi.org/10.1051/0004-6361/201936581

  • Publications
    3D thermal modeling of two selected regions on comet 67P and comparison with Rosetta/MIRO measurements

    Macher, W., Kömle, N., Skorov, Y., Rezac, L., Kargl, G., & Tiefenbacher, P. (2019). 3D thermal modeling of two selected regions on comet 67P and comparison with Rosetta/MIRO measurements. Astronomy and Astrophysics, 630, A12. https://doi.org/10.1051/0004-6361/201834798

  • Publications
    Ca II H&K stellar activity parameter: A proxy for extreme ultraviolet stellar fluxes

    Sreejith, A. G., Fossati, L., Youngblood, A., France, K., & Ambily, S. (2020). Ca II H&K stellar activity parameter: A proxy for extreme ultraviolet stellar fluxes. Astronomy and Astrophysics, 644, A67. https://doi.org/10.1051/0004-6361/202039167

  • Publications
    Size-dependent charging of dust particles in protoplanetary disks. Can turbulence cause charge separation and lightning?

    Balduin, T., Woitke, P., Jørgensen, U. G., Thi, W.-F., & Narita, Y. (2023). Size-dependent charging of dust particles in protoplanetary disks. Can turbulence cause charge separation and lightning? Astronomy and Astrophysics, 678, A192. https://doi.org/10.1051/0004-6361/202346442