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  • Publikationen
    MINDS. JWST/MIRI reveals a dynamic gas-rich inner disk inside the cavity of SY Cha

    Schwarz, K., Henning, T., Christiaens, V., Gasman, D., Samland, M., Perotti, G., Jang, H., Grant, S., Tabone, B., Morales-Calderón, M., Kamp, I., Dishoeck, E., Güdel, M., Lagage, P., Barrado, D., Garatti, A., Glauser, A., Ray, T., Vandenbussche, B., ... Temmink, M. (2024). MINDS. JWST/MIRI reveals a dynamic gas-rich inner disk inside the cavity of SY Cha. Astrophysical Journal, 962, 8. https://doi.org/10.3847/1538-4357/ad1393

  • Publikationen
    Prompt sky localization of compact binary sources using a meshfree approximation

    Pathak, L., Munishwar, S., Reza, A., & Sengupta, A. (2024). Prompt sky localization of compact binary sources using a meshfree approximation. Physical Review D, 109, 024053. https://doi.org/10.1103/PhysRevD.109.024053

  • Publikationen
    Hydrocarbon chemistry in the inner regions of planet-forming disks

    Kanwar, J., Kamp, I., Woitke, P., Rab, C., Thi, W., & Min, M. (2024). Hydrocarbon chemistry in the inner regions of planet-forming disks. Astronomy and Astrophysics, 681, A22. https://doi.org/10.1051/0004-6361/202346262

  • Publikationen
    The evaporation of planetary atmospheres

    Guenther, E., Fossati, L., & Kabáth, P. (2024). The evaporation of planetary atmospheres. Contributions of the Astronomical Observatory Skalnate Pleso, 54, 157-163. https://doi.org/10.31577/caosp.2024.54.2.157

  • Publikationen
    AESOPUS 2.0: Low-temperature opacities with solid grains

    Marigo, P., Woitke, P., Tognelli, E., Girardi, L., Aringer, B., & Bressan, A. (2024). AESOPUS 2.0: Low-temperature opacities with solid grains. Astrophysical Journal, 960, 18. https://doi.org/10.3847/1538-4357/ad0898

  • Publikationen
    Scalar-potential mapping of the steady-state magnetosheath model

    Narita, Y., Schmid, D., & Toepfer, S. (2024). Scalar-potential mapping of the steady-state magnetosheath model. Annales Geophysicae, 42, 79-89. https://doi.org/10.5194/angeo-42-79-2024

  • Publikationen
    The GAPS programme at TNG. LX. Atmospheric characterisation of KELT-9 b via single-line analysis: Detection of six H I Balmer lines, Na I, Ca I, Ca II, Fe I, Fe II, Mg I, Ti II, Sc II, and Cr II

    Arpa, M., Saba, A., Borsa, F., Fossati, L., Micela, G., Maio, C., Stangret, M., Tripodo, G., Affer, L., Bonomo, A., Benatti, S., Brogi, M., Fardella, V., Lanza, A., Guilluy, G., Maldonado, J., Mantovan, G., Nascimbeni, V., Pino, L., ... Lorenzi, V. (2024). The GAPS programme at TNG. LX. Atmospheric characterisation of KELT-9 b via single-line analysis: Detection of six H I Balmer lines, Na I, Ca I, Ca II, Fe I, Fe II, Mg I, Ti II, Sc II, and Cr II. Astronomy and Astrophysics, 690, A237. https://doi.org/10.1051/0004-6361/202449341

  • Publikationen
    Lower‐hybrid wave‐induced plasma mixing related to Kelvin‐Helmholtz vortices during southward IMF

    Blasl, K., Settino, A., Nakamura, R., Hasegawa, H., Nakamura, T., & Hosner, M. (2024). Lower‐hybrid wave‐induced plasma mixing related to Kelvin‐Helmholtz vortices during southward IMF. Journal of Geophysical Research: Space Physics, 129, e2024JA033152. https://doi.org/10.1029/2024JA033152

  • Publikationen
    Why heterogeneous cloud particles matter. Iron-bearing species and cloud particle morphology affect exoplanet transmission spectra

    Kiefer, S., Samra, D., Lewis, D., Schneider, A., Min, M., Carone, L., Decin, L., & Helling, C. (2024). Why heterogeneous cloud particles matter. Iron-bearing species and cloud particle morphology affect exoplanet transmission spectra. Astronomy and Astrophysics, 690, A244. https://doi.org/10.1051/0004-6361/202450526

  • Publikationen
    Measurement of the Taylor microscale and the effective magnetic Reynolds number in the solar wind with Cluster

    Roberts, O., Klein, K., Vörös, Z., Nakamura, R., Li, X., Narita, Y., Schmid, D., Bandyopadhyay, R., & Matthaeus, W. (2024). Measurement of the Taylor microscale and the effective magnetic Reynolds number in the solar wind with Cluster. Journal of Geophysical Research: Space Physics, 129, e2024JA032968. https://doi.org/10.1029/2024JA032968