Publicaciones en colaboración con investigadores/as de Universidad Autónoma de Madrid (14)

2010

  1. Europa: New horizons for astrobiology

    Astrobiology: Physical Origin, Biological Evolution and Spatial Distribution (Nova Science Publishers, Inc.), pp. 193-204

  2. Structural evolution of Lavinia Planitia, Venus: Implications for the tectonics of the lowland plains

    Icarus, Vol. 206, Núm. 1, pp. 210-228

  3. The present-day thermal state of Mars

    Icarus, Vol. 207, Núm. 2, pp. 631-637

2009

  1. Ancient heat flow and crustal thickness at Warrego rise, Thaumasia highlands, Mars: Implications for a stratified crust

    Icarus, Vol. 203, Núm. 1, pp. 47-57

  2. Europa: New horizons for astrobiology

    Space Exploration Research (Nova Science Publishers, Inc.), pp. 519-529

  3. New evidence for a magmatic influence on the origin of Valles Marineris, Mars

    Journal of Volcanology and Geothermal Research, Vol. 185, Núm. 1-2, pp. 12-27

  4. The geology of the venusian plains

    Space Exploration Research (Nova Science Publishers, Inc.), pp. 499-517

  5. The very early thermal state of Terra Cimmeria: Implications for magnetic carriers in the crust of Mars

    Icarus, Vol. 203, Núm. 2, pp. 454-459

2007

  1. Thermal diapirism and the habitability of the icy shell of Europa

    Origins of Life and Evolution of the Biosphere, Vol. 37, Núm. 3, pp. 287-295

2005

  1. Estimating the effective elastic thickness of the lithosphere of the Iberian peninsula based on multitaper spectral analysis

    Geophysical Journal International, Vol. 160, Núm. 2, pp. 729-735

  2. Seas under ice: Stability of liquid-water oceans within icy worlds

    Earth, Moon and Planets, Vol. 97, Núm. 1-2, pp. 79-90

2004

  1. Prime candidate sites for the astrobiological exploration of Mars according to its hydrogeological history

    European Space Agency, (Special Publication) ESA SP

  2. Prime candidate sites for the astrobiological exploration of mars according to its hydrogeological history

    PROCEEDINGS OF THE III EUROPEAN WORKSHOP ON EXO-ASTROBIOLOGY

  3. Should paleoshorelines of ancient martian oceans be close to present-day equipotential surfaces?

    European Space Agency, (Special Publication) ESA SP