About exobiology: the case for dwarf K stars |
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Acoustic heating models for the basal flux star {tau} Ceti including time-dependent ionization: results for Ca II and Mg II emission |
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Acoustic heating of the solar chromosphere: present indeed and locally dominant |
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Acoustic wave propagation in the solar atmosphere. IV. Nonadiabatic wave excitation with frequency spectra |
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The advection of supergranules by the sun's axisymmetric flows |
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Application of the Titius-Bode rule to the 55 Cancri system: Tentative prediction of a possibly habitable planet |
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Basal chromospheric flux and Maunder Minimum-type stars: the quiet-Sun chromosphere as a universal phenomenon |
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The basal chromospheric Mg ii h+k flux of evolved stars: probing the energy dissipation of giant chromospheres |
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Basal heating in main-sequence stars and giants: results from monochromatic acoustic wave models |
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Can Planets Exist in the Habitable Zone of 55~Cancri? |
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Chromospheres, flares and exoplanets |
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Chromospheric heating by acoustic shocks: a confrontation of GHRS observations of alpha Tauri (K5 III) wih AB initio calculations |
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Chromospheric velocity fields in {alpha} Orionis (M2 Iab) generated by stochastic shocks |
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The CO/SiO radiative instability in cool star atmospheres revisited |
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A critical test of empirical mass loss formulas applied to individual giants and supergiants |
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Definition and significance of average temperatures in time-dependent solar chromosphere models |
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Fitting formulae and constraints for the existence of S-type and P-type habitable zones in binary systems |
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Further results of TiO-band observations of starspots |
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Generation of extended chromospheres and mass loss of late-type giant stars due to acoustic shock waves |
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Generation of longitudinal flux tube waves in theoretical main-sequence stars: effects of model parameters |
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Generation of mass loss in K giants: the failure of global oscillation modes and possible implications |
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The great oxidation of Earth's atmosphere: contesting the yoyo model via transition stability analysis |
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Habitability of earth-mass planets and moons in the Kepler-16 system |
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The habitability of super-Earths in Gliese 581 |
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Habitability of the Goldilocks planet Gliese 581g: results from geodynamic models |
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The habitable zone of Earth-mass planets around 47 UMa: results for land and water worlds |
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The habitable zone of Kepler-16: impact of binarity and climate models |
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The heating of solar magnetic flux tubes. I. Adiabatic longitudinal tube waves |
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How Much Climatic Information Do Water Isotopes Contain? |
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A hydrodynamic code for the treatment of late-type stellar wind flows based on the method of characteristics |
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The instability transition for the restricted 3-body problem. III. The lyapunov exponent criterion |
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Line profile variations in M giants: clues to mass-loss and chromospheric heating mechanisms |
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The Mass–Luminosity Relation for a Refined Set of Late-K/M Dwarfs |
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A method for the treatment of supergranulation advection by giant cells |
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A new version of Reimers' law of mass loss based on a physical approach |
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On stellar activity enhancement due to interactions with extrasolar giant planets |
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On the validity of the "Hill radius criterion" for the ejection of planets from stellar habitable zones |
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Orbital Stability of Planet-hosting Triple-star Systems according to Hill: Applications to Alpha Centauri and 16 Cygni |
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Orbital stability of terrestrial planets inside the habitable zones of extrasolar planetary systems |
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Planet-Induced Emission Enhancements in HD 179949: Results from McDonald Observations |
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Properties of longitudinal flux tube waves. II. Limiting shock strength behavior |
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Radiative transfer in ab-initio chromospheric models |
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S-TYPE ANDP-TYPE HABITABILITY IN STELLAR BINARY SYSTEMS: A COMPREHENSIVE APPROACH. I. METHOD AND APPLICATIONS |
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A search for Ca II emission enhancement in stars resulting from nearby giant planets |
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The Secret Lives of Cepheids: {delta} Cep-the prototype of a new class of pulsating X-ray variable stars |
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Self-consistent and time-dependent magnetohydrodynamic chromosphere models for magnetically active stars |
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Shock formation of slow magnetosonic waves in coronal plumes |
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The shock strength in super- and hypergiant atmospheres derived from micro turbulence data |
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Short-term chromospheric variability in {alpha} Tauri (K5 III): results from IUE time series observations |
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Solar magnetic flux tube simulations with time-dependent ionization |
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Solar Rossby wave ``hills'' identified as supergranules |
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The stability of the suggested planet in the {nu} Octantis system: a numerical and statistical study |
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Stochastic shock waves as a candidate mechanism for the formation of the He I lambda 10830 line in cool giant stars |
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Stringent criteria for stable and unstable planetary orbits in stellar binary systems |
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Supergranule superrotation identified as a projection effect |
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Theoretical studies of comets in the 55 Cancri system |
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Time-dependent effects of acoustic wave heating and molecular cooling in the outer atmosphere of Arcturus |
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Two-component theoretical chromosphere models for K dwarfs of different magnetic activity: exploring the Ca II emission-stellar rotation relationship |
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Updated Studies on Exomoons in the HD 23079 System |
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Wave pressure in stellar atmospheres due to shock wave trains |
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What can HST-GHRS Fe II observations of {alpha} Orionis (M2 Iab) tell us about short-period heating? |
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X-ray Activity on the Star-Planet Interaction Candidate HD 179949 |
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