Migrating neptune-class bodies as a source of large terrestrial planets

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 539, 2003, Pages 491-496

  Lammer, H ^a   Selsis, F ^b   Ribas, I ^c,d   Lichtenegger, H I M ^a   Penz, T ^a,e   Guinan, E F ^d   Bauer, S J ^e   Weiss, W W ^f  

^a Austrian Academy of Sciences   (Austria)

^b CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^c UNIVERSITY OF BARCELONA   (Spain)

^d VILLANOVA UNIVERSITY   (United States)

^e UNIVERSITY OF GRAZ   (Austria)

^f UNIVERSITY OF VIENNA   (Austria)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; HYDRODYNAMICS; HYDROGEN; IONS; MATHEMATICAL MODELS; PLANETS;

ATMOSPHERIC STABILITY; EXOPLANETS; THERMOSPHERES;

ASTRONOMY;

EID: 3142699406     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

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