Fig. 3 from Plasma and Magnetic Field Parameters in the Vicinity of Short‐periodic Giant Exoplanets

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Plasma and Magnetic Field Parameters in the Vicinity of Short‐periodic Giant Exoplanets

Authors: N. V. Erkaev, T. Penz, H. Lammer, H. I. M. Lichtenegger, H. K. Biernat, P. Wurz, J.-M. Grießmeier, and W. W. Weiss

Erkaev et al. 2005 The Astrophysical Journal Supplement Series 157 396.

Provider: AAS Journals

Caption: Fig. 3.

Eccentricity of the orbits of HD 108147b and HD 162020b and the magnetosonic Mach number. The dotted line separates the region where bow shocks occur from the region without bow shocks, while the thin solid lines indicate the eccentricity of the exoplanetary orbits.

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