Mass loss from "Hot Jupiters"-Implications for CoRoT discoveries, Part II: Long time thermal atmospheric evaporation modeling

Planetary and Space Science

Volumn 56, Issue 9, 2008, Pages 1260-1272

  Penz, T ^a   Erkaev, N V ^b   Kulikov, Yu N ^c   Langmayr, D ^d   Lammer, H ^d   Micela, G ^a   Cecchi Pestellini, C ^g   Biernat, H K ^d,e   Selsis, F ^f   Barge, P ^h   Deleuil, M ^h   Leger A ⁱ  

^a INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^b INSTITUTE OF COMPUTATIONAL MODELING   (Russian Federation)

^c POLAR GEOPHYSICAL INSTITUTE   (Russian Federation)

^d University of Graz ^*  (Austria)

^e UNIVERSITY OF GRAZ   (Austria)

^f UNIVERSITÉ DE LYON   (France)

^g INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^h OBSERVATOIRE DE MARSEILLE   (France)

ⁱ UNIVERSITÉ PARIS SUD   (France)

Author keywords

Atmospheric evolution; CoRoT; Exoplanets; Hydrodynamic modeling; Mass loss; Roche lobe

Indexed keywords

ASTROPHYSICS; ATMOSPHERICS; COMPUTER NETWORKS; FLUID MECHANICS; FUNCTION EVALUATION; HYDRODYNAMICS; HYDROGEN; INDUSTRIAL ECONOMICS; MICROFLUIDICS; NONMETALS; THERMAL EVAPORATION; WIND EFFECTS; WIND POWER;

(MIN ,MAX ,+) FUNCTIONS; ABSORBED ENERGY; ATMOSPHERIC MASS LOSS; HEATING EFFICIENCY; HOT JUPITERS; HYDRODYNAMIC EQUATIONS; LONG TIME; MASS LOSSES; MAXIMUM TEMPERATURE; NUMERICAL ALGORITHMS; TIME-DEPENDENT;

FLUID DYNAMICS;

EID: 46049117473     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2008.04.005     Document Type: Article

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