June 24, 2014

Publications related to the theoretical studies (atmospheres, star-planet interactions, dynamics...)

Publications related to the theoretical studies (atmospheres, star-planet interactions, dynamics...)

Optical Flux from Hot Jupiters: Application to Kepler and CoRoT,
Fortney, Jonathan J.; Marley, M. S.; Saumon, D.; Lodders, K.; Freedman, R.,
American Astronomical Society, DPS meeting #40, #11.01; Bulletin of the American Astronomical Society, Vol. 40, p.401, 2008DPS....40.1101F

Mass loss from "Hot Jupiters"—Implications for CoRoT discoveries, Part II: Long time thermal atmospheric evaporation modeling,
Penz, T.; Erkaev, N. V.; Kulikov, Yu. N.; Langmayr, D.; Lammer, H.; Micela, G.; Cecchi-Pestellini, C.; Biernat, H. K.; Selsis, F.; Barge, P.; et al.,
Planetary and Space Science, Volume 56, Issue 9, p. 1260-1272, doi:10.1016/j.pss.2008.04.005

Mass loss of "Hot Jupiters"—Implications for CoRoT discoveries. Part I: The importance of magnetospheric protection of a planet against ion loss caused by coronal mass ejections,
Khodachenko, M. L.; Lammer, H.; Lichtenegger, H. I. M.; Langmayr, D.; Erkaev, N. V.; Grießmeier, J.-M.; Leitner, M.; Penz, T.; Biernat, H. K.; Motschmann, U.; Rucker, H. O.,
Planetary and Space Science, Volume 55, Issue 5, p. 631-642, doi:10.1016/j.pss.2006.07.010

Theoretical planetary mass spectra - a prediction for CoRoT,
Broeg, C.,
Monthly Notices of the Royal Astronomical Society: Letters, Volume 377, Issue 1, pp. L44-L48, doi:10.1111/j.1745-3933.2007.00300.x

Properties of the short period CoRoT-planet population II: The impact of loss processes on planet masses from Neptunes to Jupiters,
Lammer, Helmut; Penz, T.; Wuchterl, G.; Lichtenegger, H. I. M.; Khodachenko, M. L.; Kulikov, Yu. N.; Micela, G.,
Submitted on 19 Jan 2007, arXiv:astro-ph/0701565v1

Properties of the short period CoRoT-planet population I: Theoretical planetary mass spectra for a population of stars of 0.8 to 2 solar masses and orbital periods of less then 20 days,
Wuchterl, G.; Broeg, C.; Krause, S.; Pecnik, B.; Schoenke, J.,
Submitted on 29 Dec 2006, arXiv:astro-ph/0701003